The galaxy presents as an elliptical morphology with a smooth, centralized bulge. The luminosity profile appears centrally concentrated, gradually decreasing outwards. The color gradient transitions from a yellow-orange core to a bluer halo, indicating the presence of a potentially older stellar population in the center, while the outer regions may contain younger, bluer stars, or enhanced metallicity. There is a subtle suggestion of faint outer structure, but no distinct spiral arms or bar are discernible. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. The shape is generally elliptical, with a slight elongation.
