The galaxy appears to be an elliptical galaxy, showing a smooth, relatively featureless morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity outward. The overall shape approximates a rounded form, with a slight deviation from perfect circularity. There is evidence of a redder hue concentrated in the core region, potentially indicating an older stellar population dominating the central bulge. The outer regions display a bluer tint, hinting at the presence of some younger stars and ongoing, albeit limited, star formation. No prominent spiral arms or bars are visible, which further corroborates its classification as an elliptical galaxy. There is a very small amount of disturbance that suggests a past merger event. The galaxy is likely undergoing a slower rate of star formation compared to spiral galaxies.