The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. There is a luminous core region, transitioning into a more diffuse halo. The light distribution suggests a high degree of rotational symmetry. The color profile indicates a relatively old stellar population, with a yellow-red hue dominating the core and inner regions, transitioning to slightly bluer tones in the outer halo. No distinct spiral arm structures are apparent, nor is there evidence of significant dust lanes or recent major mergers. Minor disturbances cannot be completely ruled out but the general appearance is quite smooth and symmetrical.
