The galaxy appears to be a disk galaxy viewed at a high inclination, nearly edge-on. There is a bright central bulge, and a faint disk extending outwards. Some asymmetry is present in the disk, but overall there are no signs of a recent major merger or tidal disruption. There may be a slight distortion in the disk on one side, which could indicate a minor merger event or gravitational interaction. The inner region of the disk shows hints of spiral arm structure, though this is hard to confirm. The galaxy exhibits a color gradient, being bluer in the disk compared to the bulge, which appears to be relatively redder. This suggests more active star formation occurring in the disk regions compared to the bulge. Overall, the galaxy seems relatively undisturbed, possibly undergoing minor interactions, and exhibiting ongoing star formation.
