The galaxy presents as a smooth, elliptical-like structure with a concentrated central bulge. The color profile indicates a likely evolved stellar population, dominated by older, redder stars, particularly in the central region. There is a slightly more bluer color towards the edge of the galaxy. The lack of prominent spiral arms or significant dust lanes supports the interpretation of an early-type galaxy. The overall morphology is very round, with little sign of tidal disturbances or ongoing major mergers. The galaxy is relatively compact in size.
