This galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a concentrated central bulge. The light profile suggests a fairly uniform distribution, indicative of an older stellar population and minimal ongoing star formation. The shape appears somewhat elongated, but is more in between round and cigar shaped. There is no evidence of tidal tails, merging features, or significant dust lanes, suggesting it is not undergoing any major interaction. Its color is somewhat on the redder side, implying the presence of evolved stars. Overall, it seems to be a fairly quiescent galaxy that is a relaxed system with no significant signs of recent disturbances.
