The galaxy appears to be a relatively smooth, elliptical galaxy. There is a bright, concentrated central bulge that dominates the overall structure. Moving outward from the bulge, the luminosity gradually decreases. The galaxy appears yellowish-white. Based on the concentration of light and lack of obvious spiral arms or dust lanes, a significant portion of its stellar population is likely older stars. There might be a very faint, diffuse disk surrounding the bulge, but it lacks significant structural features. There is no evidence of any major merging events or tidal disturbances, although there is some indication of a slight asymmetry in the outer regions which might be from a minor disturbance.