The galaxy presents a largely smooth morphology. The light distribution is dominated by a central bulge with a high degree of circularity. There is a faint, extended halo surrounding the central region. Weak disk-like features might be present. There is no strong evidence of spiral arm structure or significant dust lanes. The galaxy appears to be relatively undisturbed with no clear signs of a major merger event. The color profile indicates a dominant population of older stars, but there is some evidence of younger stars present in a small population within the galaxy.
