The galaxy presents as a relatively smooth, elliptical or lenticular structure. Its central region is characterized by a bright, concentrated bulge, exhibiting a yellowish-white hue, suggestive of an older stellar population. The outer regions display a more diffuse and fainter envelope, blending gradually into the background sky. There is no discernible spiral arm structure. The overall shape appears mostly round. There are no obvious signs of major interaction or merging activity, although there may be a slight asymmetry indicating minor disturbances.
