The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, with a gradual decrease in luminosity towards its periphery. There is little evidence of distinct spiral arms or a prominent disk-like structure. The primary color of the galaxy is a yellow/orange hue, suggesting a population of older stars, although there appears to be some blue tint in the surrounding area that might indicate some recent star formation. The overall roundness suggests a classification leaning towards an elliptical galaxy. There is no obvious sign of tidal disturbances or a merging event. The galaxy appears relatively isolated and undisturbed.
