The galaxy exhibits an elliptical morphology. It possesses a smooth, centrally concentrated bulge that dominates the overall light distribution. The bulge appears yellowish-orange in color, suggesting a population of older stars.

A faint, reddish ring-like structure is observed surrounding the central bulge. This feature could indicate recent or ongoing star formation within a disk-like component. The galaxy is elongated, with a clear major axis and a less prominent minor axis. The light distribution is not perfectly smooth, showing some subtle irregularities. These irregularities might point to minor interactions or internal dynamical processes.
