The galaxy presents as a moderately bright, fairly regular elliptical or lenticular system. A bright, relatively homogenous central bulge dominates the morphology. This core region is a pale yellow-white. Extending outward from the center, a more diffuse halo can be observed. The halo is subtly elongated along a major axis. No distinct spiral arm structure is discernible. The overall color of the halo appears slightly redder than the core. There is a subtle hint of a possible disk. There is no evidence of active star formation. There may be some signs of minor past tidal disturbances.
