The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. Its color profile suggests an older stellar population, characterized by a yellowish-red hue towards the core. There is no readily apparent spiral structure or significant dust lane obscuration. The overall texture is relatively uniform with a high degree of smoothness. There are subtle color variations in the galaxy's halo. The isophotes appear mostly regular and lack any signs of major tidal disturbances or ongoing merging activity.
