The galaxy presents a generally smooth and concentrated morphology. It appears elliptical in shape, with a high degree of central concentration and a gradual decrease in luminosity towards the outer edges. The core region exhibits a yellowish hue, suggesting an older stellar population. There is very little evidence of distinct spiral arms or significant dust lanes. Faint color variations are present in the outer regions but it is difficult to determine if it corresponds to recent star formation. Overall, the galaxy's light profile is consistent with an early-type galaxy undergoing limited star formation. The overall appearance indicates a system that has likely undergone significant evolutionary processes, resulting in a relatively quiescent state.
