The galaxy presents as a single, well-defined object with a smooth, elliptical morphology. It exhibits a concentrated central bulge that appears near-spherical. The color gradient suggests an older stellar population dominating the galaxy's composition, with a yellower/redder hue in the core region, indicating a concentration of evolved stars. No distinct spiral arms or disk-like structures are discernible. There is no obvious evidence of active star formation within the galaxy, and the overall structure lacks features indicating a recent major merger event, although a minor disturbance cannot be ruled out. The galaxy is likely a quiescent, early-type galaxy with a substantial stellar mass.
