The galaxy presents as a relatively smooth, centrally concentrated object. It displays a yellowish-white hue, suggestive of an older stellar population. The galaxy appears to be mostly elliptical in shape with a small irregularity that could suggest minor tidal disturbances or an ongoing merger with a smaller object. It exhibits a notable central bulge that fades into a more diffuse halo. The overall structure suggests a late-type spiral or lenticular galaxy viewed at a considerable distance, with very little ongoing star formation.
