The galaxy presents as a moderately luminous, elliptical or lenticular system. It exhibits a smooth, centrally concentrated light profile, with the highest intensity concentrated toward the core, gently fading outwards. There is a slight elongation, appearing more cigar-shaped than perfectly circular, but with no prominent bar structure. The central region appears yellowish-white, implying an older stellar population. Faint hints of bluer star formation regions are visible in the outer regions and along one edge of the disk. These regions are not well-defined. There is no obvious evidence of major disturbances or ongoing mergers, although very subtle distortions are present in the outer halo of the galaxy, this galaxy exhibits little to no spiral arm structure. Its integrated color suggests a relatively evolved stellar population.
