The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a smooth, centrally concentrated morphology. The dominant feature is a bright, yellowish bulge. Little to no resolved spiral arm structure is discernible. The galaxy is somewhat flattened, and not perfectly spherical. There are no obvious signs of tidal disturbances or major merger activity. Faint, diffuse light extends from the central bulge, suggesting a stellar halo, though its extent is difficult to discern. The galaxy's color indices, based on observed g, r, and z bands, suggest a population of older stars and a low rate of on-going star formation. The overall appearance is consistent with a relatively evolved system.
