The object presents as a merging or interacting galaxy system. It is comprised of two primary galactic nuclei, with the overall morphology being significantly disturbed. Both nuclei exhibit high luminosity. A faint, diffuse halo surrounds the central region, suggesting tidal interactions and a potential starburst phase triggered by the merger. There is an extended, distorted disk or tidal tail structure emanating from the main body, indicating gravitational disruption. The object’s color index suggests a mix of stellar populations, with a possible presence of younger, bluer stars formed during the interaction and older, redder stars in the existing galactic structures. The dust lanes are obscured, indicating this is a more intermediate stage merger, or a face-on viewing angle.
