The galaxy appears as a luminous, somewhat centrally concentrated object. It exhibits a dominant, smooth component. The overall shape is elliptical, appearing nearly round, with no strong deviations from circular symmetry discernible at this resolution. There is no obvious spiral structure. The galaxy's color is slightly redder, consistent with an older stellar population. There is no obvious evidence of major ongoing mergers or strong tidal distortions but there may be minor disturbances.
