The galaxy exhibits a generally smooth, elliptical morphology. The central region presents a bright, concentrated luminosity, suggestive of a prominent galactic nucleus. Moving outwards, the luminosity gradually decreases into a more diffuse halo.

The overall color is relatively red, implying an older stellar population with reduced ongoing star formation. There is a subtle hint of bluer light in a small area of the galaxy, potentially indicating some residual star formation.

The shape is largely spheroidal, with minimal indication of a disk-like structure. The overall impression is of a mature, relatively quiescent galaxy. There are no obvious signs of significant tidal disturbances or ongoing mergers.
