The galaxy appears as a diffuse, elliptical-shaped object. Its core exhibits a strong concentration of light, suggesting a substantial stellar population or possibly an active galactic nucleus. Moving outward from the core, the luminosity decreases gradually. No distinct spiral arms or a bar structure are discernible. The overall color is yellowish, indicating a relatively older stellar population. The galaxy exhibits a smooth texture, and no significant dust lanes or patches of intense star formation are obvious. There are no signs of ongoing major mergers or tidal disturbances.
