The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that transitions smoothly into a diffuse halo. There is little indication of spiral arm structure or prominent dust lanes. The overall color appears to be yellowish-orange, suggestive of an older stellar population. It has a slight elongation in its shape, but is mostly round. There are no immediately obvious signs of ongoing mergers or major tidal disturbances. The galaxy appears relatively isolated.
