The galaxy presents as a relatively smooth, elliptical-like structure with a high degree of circularity. There is a subtle color gradient visible, with a slightly bluer hue in the central region transitioning to redder tones in the outer regions of the galaxy. No obvious spiral arms or distinct features of a disk galaxy are apparent. Overall, the galaxy exhibits a relaxed morphology, with no indications of ongoing major mergers or significant tidal disturbances. It has an estimated size of approximately 7 kiloparsecs. The galaxy's estimated mass is significant, suggesting a substantial population of stars and potentially a supermassive black hole at its center. Based on colors, star formation is moderate but ongoing. 
