The galaxy presents as a relatively smooth and featureless elliptical. It exhibits a concentrated central bulge that gradually fades into an extended halo. The color profile suggests a mature stellar population, with a dominant yellow-orange hue. There are some hints of what may be faint spiral arm remnants or tidal streams, but there is no significant presence of dust lanes. There is no obvious indication of a recent major merger. The galaxy has a moderate to high mass, and a relatively low star formation rate.