This galaxy presents as a relatively smooth, elliptical or lenticular system, exhibiting a high degree of central concentration. The light is dominated by older stellar populations, resulting in a yellow-red hue. There is little indication of prominent spiral arms or significant dust lanes. The galaxy appears quite regular in shape, lacking obvious signs of major mergers or tidal distortions. The isophotes appear largely elliptical and symmetrical. Slight indications of extended low surface brightness features may be present, however, these are quite faint and difficult to ascertain. The lack of pronounced features suggests a relatively quiescent galaxy, where star formation has either ceased or is proceeding at a low rate.
