The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth morphology. The core exhibits a bright, yellowish-white hue, suggestive of a significant population of older stars. The light distribution appears relatively even, with a high degree of central concentration. The overall shape is slightly elongated, deviating somewhat from a perfect circle. There is minimal evidence of spiral arms or significant dust lanes, indicating a lack of prominent ongoing star formation. A faint, diffuse halo surrounds the central region, gradually fading into the background sky. No obvious signs of tidal disturbances or mergers are apparent, indicating that this galaxy may have been relatively undisturbed for a long period. The color profile suggests that star formation is very low to negligible.
