The galaxy presents as a single, relatively smooth, and concentrated object. It exhibits a near-spherical morphology, lacking any apparent spiral arms or significant disk-like features. The central region appears brighter and more concentrated than the outer edges, suggesting a dominant bulge component or a centrally located active galactic nucleus. The overall color appears yellowish-red, potentially indicating an older stellar population, or significant dust reddening within the galaxy. There is no obvious tidal debris or merging companion, suggesting it is not currently undergoing a major interaction. However, there seems to be some very minimal disturbance, possibly caused by a minor interaction.