The galaxy presents as a relatively smooth, elliptical-like structure. Its overall color is a yellowish-white, suggesting a population of older stars. There is some indication of a slight blue tint in the outer regions, potentially indicating the presence of some younger, hotter stars, though this is marginal. The galaxy appears primarily spheroidal in shape, with no obvious spiral arms or a significant disk component visible. There are no signs of any major ongoing merger events or tidal disturbances in the main body of the galaxy. It displays a concentrated central bulge and a gradual decrease in surface brightness towards the outer regions. 
