The galaxy presents as a fairly smooth, elliptical-like object with a concentrated central bulge. The color gradient suggests an older stellar population, with a yellowish-orange hue dominating the central regions, potentially indicating a lack of significant recent star formation. The galaxy is mostly round. There are possibly minor asymmetries or disturbances in the outer regions, which may be indicative of minor gravitational interactions or past merger events, though this is not clearly distinguished.
