This galaxy presents as a slightly elongated, elliptical-like structure with a smooth, diffuse light distribution. The core region exhibits a yellowish-white hue, suggestive of an older stellar population dominating the central bulge. The light intensity gradually decreases from the center outwards, indicating a higher stellar density towards the core. There is a subtle color gradient from the center, with the outer regions appearing slightly bluer. Overall, the galaxy appears to be in a relatively quiescent state, with minimal signs of active star formation or significant dust lanes. Based on its morphology, it appears as though it has a very faint disk. There are no indications of any major ongoing merging activity or significant tidal disturbances.