The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears to be the brightest region of the galaxy. Proceeding outwards from the core, the luminosity decreases. The galaxy is not perfectly circular, as it appears elongated along one axis, but it has fairly uniform coloration. There are no discernible dust lanes or spiral arms. The overall color suggests an older stellar population. The galaxy does not seem to be undergoing any major mergers or tidal disturbances, and it looks relatively isolated and unperturbed.
