The galaxy presents as a generally smooth, centrally concentrated object. It exhibits an elliptical morphology with a high degree of roundness. A central bulge is evident, displaying a yellowish-orange hue, which suggests an older stellar population. There is a subtle color gradient outwards from the center, with the outer regions exhibiting a slightly bluer tint, potentially indicating the presence of younger stars or a small amount of on-going star formation. There is no clear evidence of spiral arms or a distinct disk structure. Overall, the galaxy appears relatively undisturbed, showing no significant signs of major mergers or tidal interactions.
