The galaxy appears to be an elliptical galaxy, exhibiting a smooth, spheroidal morphology with no discernible spiral arm structure. Its color gradient suggests an older stellar population, with a yellowish hue dominating the central region, potentially indicating a lack of ongoing significant star formation. The galaxy presents a well-defined core with a gradual decrease in luminosity towards its outer edges, suggesting a concentration of stars and a likely supermassive black hole at its center. There are no signs of any major ongoing mergers or significant tidal disturbances.
