The galaxy presents as a largely smooth, elliptical-like structure. It exhibits a moderate degree of ellipticity, appearing more elongated than perfectly spherical. There is a central concentration of light, suggesting a nucleus. The light tapers off gradually outwards from the center of the galaxy. There appears to be a relatively low level of current star formation, with subtle colour variations and lack of well-defined spiral arms. Subtle irregularities in the outer regions suggest possible past interactions or minor disturbances. Overall, the galaxy displays characteristics consistent with a relatively evolved system.
