The galaxy appears as a centrally concentrated, smooth object, with a largely elliptical morphology. Its color profile indicates a possible red sequence galaxy. The light is most intense towards the center, becoming fainter outwards. The structure is dominated by a spheroidal component, with no apparent spiral arms or a pronounced disk. There are no obvious signs of recent or ongoing major merger activity. The overall visual impression is of a mature system with little discernible substructure within the galaxy.
