The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing mostly round with a slight tendency towards being in between round and elongated. The color profile suggests a dominant population of older stars, indicated by the redder central regions, while the surrounding regions are slightly bluer. There's a lack of significant spiral arm structure or prominent dust lanes, reinforcing the classification as a likely elliptical galaxy. A small fraction may have been disturbed by minor merging events.