The galaxy presents as a centrally concentrated, relatively smooth, and luminous object. Its morphology appears largely elliptical or lenticular, exhibiting a high degree of radial symmetry. The light distribution is centrally peaked, indicating a substantial bulge component. There are no discernible spiral arm features or prominent dust lanes. The galaxy exhibits a yellowish-white hue, indicative of a population of older stars with relatively little ongoing star formation. The small angular size suggests a relatively small physical extent. There is no obvious evidence of any major ongoing mergers or tidal disturbances, although subtle irregularities could potentially indicate a minor interaction.
