The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits a yellowish-orange hue, suggestive of an older stellar population dominated by redder stars. There is no apparent spiral structure or significant dust lanes visible in the image. The galaxy appears fairly round in shape, with only a slight elongation. The overall morphology indicates a galaxy that has likely undergone significant evolution and possibly represents a system where star formation is currently suppressed or occurring at a low rate. The size of the galaxy is consistent with a large galaxy. No signs of tidal disturbances or ongoing mergers are discernible.
