The galaxy presents a smooth, elliptical morphology. It exhibits a concentrated central bulge, characterized by a yellowish hue, suggesting a population of older stars. The outer regions of the galaxy display a fainter, more diffuse halo with a slightly bluer color, possibly indicating a younger stellar population. There is a subtle hint of a disk structure, but it is not prominently defined. Overall, the galaxy appears to be relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions.