The galaxy presents as a relatively compact system. The overall form appears elliptical in shape, with a moderate degree of elongation. The light distribution is centrally concentrated, displaying a smooth, though not entirely uniform, profile. There is little discernible substructure or features typically associated with spiral arms or significant dust lanes. Its color is predominantly redder, potentially indicating an older stellar population and lower current star formation rate. There are no obvious signs of major mergers, though minor disturbances cannot be ruled out based on this image alone. The projected size of the galaxy suggests it is a moderately sized system.
