The galaxy presents as a relatively smooth, elliptical-like structure with a bright central bulge. There appears to be a very faint, diffuse halo surrounding the central region, indicating the possible presence of older stellar populations extending outwards. The primary color of the galaxy is slightly yellowish, suggesting a population dominated by older, redder stars. There may be faint hints of a very thin disk like feature, but it does not dominate the overall structure. Distortions are minimal, suggesting it is either not currently undergoing a major merger event or is in the later stages of a past minor merger. The galaxy appears to be relatively isolated in this field. Star formation rate seems to be low.
