The galaxy appears as a moderately compact, elliptical-type system, generally smooth in texture, with a slight elongation. It displays a relatively concentrated core region which decreases outward. A small amount of disturbance could be present, but it is subtle. The overall color suggests a population of older stars, with a bias towards the redder end of the spectrum. Star formation activity appears to be present, but very faint. The galaxy is approximately 10.98 kpc in radius.
