The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth, diffuse profile. A notable color gradient is observed, transitioning from a bright, yellow-white core to a more subdued, reddish-yellow outer halo. No distinct spiral arms or prominent dust lanes are apparent. The overall morphology appears undisturbed, showing no obvious signs of recent major mergers or significant tidal interactions. The light distribution suggests a high degree of rotational symmetry, with a near-circular shape.
