The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. Its overall color index suggests a population of older stars, potentially with a low ongoing star formation rate. The galaxy appears relatively undisturbed, showing no signs of major mergers or significant tidal interactions. The primary light is yellowish-white in color, becoming slightly more orange at the core. The galaxy exhibits a small apparent size, suggesting a moderate distance. There is some irregularity in the isophotes, but it appears to be largely spheroidal. A possible minor disturbance can be inferred from a slight asymmetry. 
