The galaxy appears to be an elliptical galaxy, characterized by a smooth, spheroidal shape. The light is concentrated towards the center with a gradual decrease in intensity outwards. It exhibits a predominantly yellowish-orange hue, suggestive of an older stellar population with fewer hot, young stars. No distinct spiral arms or a prominent disk structure are visible. There are no signs of ongoing or recent major merging events. The galaxy appears relatively undisturbed.
