The galaxy presents as a somewhat elliptical, yet largely featureless, object. A central, brighter region suggests a galactic nucleus, surrounded by a more diffuse halo. The galaxy exhibits a smooth, lenticular appearance. There is minimal evidence of spiral arm structure or dust lanes within this resolution. The color gradient indicates a potentially aging stellar population. There are no readily apparent signs of tidal disturbances or mergers occurring. The light distribution appears to be consistent with a de Vaucouleurs profile.
