The galaxy presents as a somewhat smooth, elliptical-like structure with a bright, concentrated central bulge. There's a noticeable color gradient, transitioning from a yellowish-white core to a reddish-orange hue in the outer regions. The galaxy appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions. It exhibits a somewhat elongated shape, not perfectly spherical, and possesses a diffuse halo extending beyond the main body of the galaxy. Based on the observed color and morphology, the stellar population likely consists predominantly of older stars, with a low rate of ongoing star formation. There is a hint of a disk-like structure, but it is faint.
