The galaxy presents as a relatively smooth, elliptical morphology with a slight elongation. A bright, concentrated central bulge dominates the structure, exhibiting a yellowish-white hue, indicative of an older stellar population. The outer regions of the galaxy gradually fade into a less defined halo, with a subtle gradient in luminosity as one moves outwards from the core. There is only the slightest hint of a disk. The galaxy appears largely undisturbed, showing no major signs of ongoing mergers or significant tidal interactions.
