The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth, concentrated structure with a high degree of circular symmetry. The color profile suggests a dominant population of older stars, indicated by the yellowish-orange hue in the central region. The light is centrally concentrated. There is little evidence of spiral arms or dust lanes. The galaxy's shape is notably round, with only a slight deviation from perfect circularity. It presents no obvious signs of major mergers or significant tidal disturbances. The overall appearance is consistent with a relatively evolved system, possibly with ongoing but moderate star formation activity.