The galaxy presents as a relatively smooth, elliptical morphology. The central bulge is bright and concentrated, exhibiting a yellowish-white hue, indicating a significant population of older stars. Moving outward from the core, the galaxy fades into a less luminous halo. The halo shows a slightly reddish tint. The galaxy appears elongated. There is some minor disturbance in the morphology. Overall, the galaxy seems to be in a relatively stable state of evolution with moderate star formation.
