The galaxy presents a generally smooth and elliptical morphology, with a high degree of central concentration. The light distribution is relatively uniform, without prominent spiral arms or distinct features. The galaxy appears somewhat round in shape. There is a subtle color gradient, appearing slightly more yellow towards the center, which could indicate a population of older stars dominating the core region. Peripheral regions seem slightly less yellow. There is no obvious indication of active merging or significant tidal disturbances in its immediate vicinity.
