The galaxy appears as a single, largely homogenous, and concentrated object. It exhibits a smooth morphology, with no visible spiral arms or distinct features typically associated with disk galaxies. The light distribution is centrally concentrated, indicating a likely spheroid shape. The color appears yellow-white, suggesting a population of older stars with a relatively low rate of star formation. There is no obvious evidence of ongoing major mergers or tidal disturbances. The galaxy is relatively compact, with a modest apparent size.
