The object presents as a merging or interacting galaxy system. There appear to be at least two distinct galactic nuclei, one exhibiting a yellower hue, and the other appearing with a bluer tint, potentially indicative of differing stellar populations. Tidal features are visibly impacting its overall structure, including distorted arms, a prominent tail, and visible dust lanes, which suggests ongoing gravitational interaction and mass transfer between the progenitor galaxies. Spiral patterns are discernible. The spiral arms appear to have tight winding, with multiple arm structures, and potentially some flocculent regions. The inner bulge appears to have a moderate size, while the bar is difficult to discern. Overall this system has a central region of moderate size, with spiral arms and potential ongoing merging or interacting. 