The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. Its color profile suggests a dominant population of older stars, evident in the yellowish-orange hue of the core region. There's a subtle decline in surface brightness moving outwards from the core. The overall structure appears largely undisturbed, lacking any signs of major mergers or significant tidal distortions. Faint, diffuse outer regions indicate the presence of a stellar halo.
