The galaxy presents as a relatively smooth, elliptical form. A bright, concentrated nucleus dominates the central region, suggesting a significant concentration of stars. The surrounding halo appears diffuse, with a gradual decrease in luminosity extending outwards from the core. There are no prominent spiral arms or disk-like structures readily visible. The overall color appears to be a yellowish-orange hue, indicating a population of older stars with fewer young, blue stars present. There is no apparent evidence of ongoing major mergers or tidal disturbances, although a slight asymmetry in the outer halo cannot be ruled out without further analysis. The galaxy exhibits a moderate degree of roundness, not appearing highly elongated or flattened.
