The galaxy presents as a primarily smooth, elliptical-like structure. It appears to be relatively undisturbed, showing no signs of major mergers or significant tidal features. The galaxy exhibits a central, highly luminous region suggestive of a dense stellar population. The shape is somewhere between perfectly round and cigar-shaped. It presents a generally smooth and regular morphology, with the bulk of the light concentrated toward the center. There is minimal evidence of spiral arm structure or prominent dust lanes. The overall color suggests an older stellar population, with a relatively weak star formation rate. A slight disturbance cannot be ruled out.