The galaxy presents as a system with a largely smooth, elliptical morphology. The light is centrally concentrated, with a prominent core. The overall shape is closer to in-between, and does not present as either particularly round or elongated. There is some evidence of a possible disk-like component, as well as light from possible recent star formation, though these are not dominant features. There does not appear to be any strong tidal features or other indications of recent major merger activity, although some minor disturbances cannot be ruled out.
