The galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a concentrated, bright core region that graduates outward into a fainter, more diffuse halo. The overall shape is somewhat elliptical. There may be a hint of a very faint, extended feature that could suggest some minor interaction or past merger event. The color profile indicates a population dominated by older stars, with a redder hue suggestive of lower star formation rates.
