The galaxy presents as a centrally concentrated object with a smooth overall morphology. It exhibits an elliptical or lenticular shape, appearing somewhat elongated rather than perfectly spherical. The light distribution suggests a relatively featureless structure, lacking prominent spiral arms or distinct bar features. There is a smooth gradient in luminosity from the bright central core outwards, indicating a gradual decrease in stellar density. The galaxy appears to be a mature system with little evidence of recent major mergers or significant tidal disturbances, although minor disturbances cannot be ruled out entirely. The color is generally yellowish, consistent with a population of older stars.
