The galaxy appears to be a single, somewhat rounded object. There is evidence of a central bulge, with a smooth, diffuse halo of light extending outwards. There is a possible hint of spiral arm structure within this halo, but the resolution is not high enough to make a conclusive determination. Color gradients are subtle, with the core appearing slightly more yellow and the outer regions exhibiting a bluer hue. This could imply ongoing star formation in the outer disk. The overall appearance suggests a galaxy that is not currently undergoing a major merger or significant tidal disruption, although the slightly irregular shape hints at past interactions or internal dynamical processes.
