The galaxy presents as a generally smooth, elliptical-like structure. Its light profile indicates a highly centrally concentrated object. It appears quite round with little to no indication of a disk-like morphology or spiral arm structures. There is no strong visual evidence of ongoing mergers or tidal disturbances in the immediate vicinity. The galaxy's color suggests a population of older stars, corresponding to a low rate of recent star formation, but there is still some light in the blue and green color bands suggesting some relatively younger stars. Overall, the galaxy appears to be a massive, relatively quiescent system.
