The galaxy presents as a centrally concentrated object, appearing largely spheroidal in shape, with a high degree of apparent smoothness. The central region exhibits a bright, yellowish-white hue, suggesting a population of older stars. Fainter, reddish tinges extend outwards from the central bulge. There are no obvious signs of strong spiral arm structures or significant dust lanes. Weak hints of asymmetry are observed, which may indicate ongoing or recent minor disturbances. This object shows no signs of currently merging with other galaxies.
