The galaxy presents as a smooth, centrally concentrated object. It is somewhat elliptical in shape, with a moderate degree of ellipticity; it is neither perfectly round nor highly elongated. The central region exhibits a bright, condensed core, likely a galactic bulge. The light profile appears to fade gradually outwards from the center. There is minimal indication of spiral arms or distinct disk-like structure. Faint asymmetries or irregularities are suggested in the outer regions, but these are not pronounced enough to indicate a major ongoing merger event, however, a potential minor disturbance might be occurring. The overall color is consistent with an older stellar population, tending towards redder wavelengths. This galaxy is likely a massive, evolved system, possibly a lenticular or elliptical galaxy. Star formation is suspected to be very low in this galaxy.
