The galaxy presents as a relatively smooth, elliptical object with a somewhat concentrated central bulge. It exhibits a predominantly yellow-orange hue, suggesting a stellar population dominated by older, redder stars, and a relatively low rate of ongoing star formation. The galaxy appears moderately massive. There is a slight elongation to its shape, though it generally appears round. There is no apparent evidence of strong tidal interactions or ongoing merging activity, though there might be very subtle, minor disturbances in the outer regions. Overall, it seems to be a relatively evolved and quiescent galaxy.
