The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge that gradually diffuses outward into a less defined halo. The color gradient suggests a population of older stars dominating the central region, indicated by the reddish-yellow hue. Fainter, bluer regions may be present within the outer regions. The overall shape is largely spheroidal, with a slight elongation. There are no apparent signs of strong tidal disturbances or major mergers.
