The galaxy presents as a generally smooth, elliptical structure. It exhibits a concentrated, bright central bulge, indicating a significant population of older stars. The color profile appears yellowish-red, which is consistent with an aging stellar population and lower rates of active star formation within the galaxy itself. There is a faint disk-like component surrounding the central bulge, appearing slightly elongated. Possible minor disturbances in the outer regions may suggest interactions with other galaxies but this is not very obvious. The galaxy appears relatively isolated in this view.