The galaxy presents as a relatively smooth elliptical or lenticular structure with a bright, somewhat concentrated central bulge. It exhibits a subtle disk-like component with a slight elongation. The primary color is a pale blue-white, possibly indicating the presence of a moderate population of younger, hotter stars, although the overall color suggests a galaxy dominated by an older stellar population. There appears to be some minor disturbance within the galactic structure, but it is not extreme. The galaxy is likely experiencing moderate star formation activity. The faint halo suggests ongoing or recent interactions, but overall, the galaxy seems relatively isolated, and its morphology is consistent with a galaxy undergoing typical, gradual evolution.
