The galaxy presents as a relatively smooth, elliptical object, with a notable central bulge that appears bright and concentrated. The overall shape is closer to being in-between round and elongated with a slight preference for a disc shape, but the apparent smoothness suggests an earlier morphological type. The galaxy does not show evidence of any major mergers or significant tidal disturbances. The color gradient suggests a population of older stars, contributing to the yellow-red hue. Star formation rates appear low. The galaxy is of significant mass, suggesting a mature system.
