3C 315 is described having a flattened appearance and a dust obscured central nucleus.[7] Its nuclear ellipticity is found to decrease at a large radius and has a central elongated structure which suggests an edge-on stellar disk.[8] It has an arc feature described as faint, which is located at a southern end of the galaxy. A large round galaxy companion is seen in the direction of south.[9] The total star forminginfrared luminosity of 3C 315 is estimated to be (1.4 ± 0.61) x 1010Lʘ.[10]
The source of 3C 315 is found peculiar with a banana-shaped radio structure.[8] When imaged, it has a central component[11] resolved into two individual components that are extended on each side of the central object. These components are however elongated and are perpendicular to the axis source. The flux density of both components at 5.0 GHz are estimated to be 1.3 ± 0.2 10−26 W m−2Hz−1.[12] The radio core is found associated with a much brighter member galaxy in the system according to Very Large Array observations.[13] A weak hotspot is seen possibly located in the northeastern arm.[14] Evidence also showed the source is found heavily polarized with the levels rising by 50% in the north point extension.[15]
Spectral index mapping using radio maps at 1.65 and 2.7 GHzfrequencies, have shown flat and steep spectral index regions located close to the core and at the tips of the radio lobes of 3C 315. Based on observations, both the northern and southern lobes have spectral indices of -1.46 and -1.26 at high frequencies, while most of the regions have a low-frequency measuring between -0.78 and -1.31. The wings located at northeast and southeast have measured spectra indices of -1.31 ± 0.03 and -1.27 ± 0.02 respectively.[5] A study published in 2024 suggested the X-shaped source of 3C 315 might be influenced through environmental factors, given the galaxy host's location inside a cluster.[16]
^ abCapetti, A.; de Ruiter, H. R.; Fanti, R.; Morganti, R.; Parma, P.; Ulrich, M.-H. (October 2000). "The HST snapshot survey of the B2 sample of low luminosity radio-galaxies: a picture gallery". Astronomy and Astrophysics. 362: 871–885. arXiv:astro-ph/0009056. Bibcode:2000A&A...362..871C. ISSN0004-6361.
^Shi, Yong; Ogle, Patrick; Rieke, George H.; Antonucci, Robert; Hines, Dean C.; Smith, Paul S.; Low, Frank J.; Bouwman, Jeroen; Willmer, Christopher (November 2007). "Aromatic Features in AGNs: Star-forming Infrared Luminosity Function of AGN Host Galaxies". The Astrophysical Journal. 669 (2): 841–861. arXiv:0707.2806. Bibcode:2007ApJ...669..841S. doi:10.1086/521594. ISSN0004-637X.
^Borka Jovanović, V.; Borka, D.; Jovanović, P. (2024-11-26). "X-shaped radio galaxy 3C 315"(PDF). BOOK OF ABSTRACTS AND CONTRIBUTED PAPERS - International Meeting on Data for Atomic and Molecular Processes in Plasmas: Advances in Standards and Modelling. Belgrade, Serbia: Institute of Physics Belgrade. pp. 30–39. doi:10.69646/aob241108. ISBN978-86-82441-69-4.
