The galaxy presents as a relatively smooth, elliptical structure. It exhibits a bright, concentrated central bulge. Fainter, diffuse light extends outward from the core, creating a halo-like appearance with a slight elongation, being neither perfectly round nor highly elongated. The central region displays a yellowish-orange hue, suggestive of an older stellar population. The outer regions show a faint blue tint, indicating the presence of some younger stars. There is no clear evidence of spiral arms or significant dust lanes.
