The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards the outer regions. The color profile indicates a dominant population of older stars, with a yellowish-orange hue at the core transitioning to a slightly bluer tint in the outskirts, suggesting minimal ongoing star formation. The overall structure appears undisturbed, showing no evidence of significant tidal interactions or recent merger events. The galaxy's shape is roughly spheroidal, with a minor deviation toward an elongated form.
