The galaxy presents a generally smooth, elliptical morphology. The light is concentrated towards the center, forming a bright, somewhat yellowish core. This suggests an older stellar population dominating the central region. The color shifts towards redder hues from the center outwards. The overall structure appears relatively undisturbed with no major asymmetries or tidal features apparent. The disk component is not easily visible, suggesting a bulge-dominated system. The galaxy exhibits a faint, diffuse halo surrounding the central region, that is composed of older stars. 