The galaxy presents a smooth, elliptical morphology. It exhibits a pronounced central bulge, bright and concentrated in the core region, which gradually fades into a more diffuse halo. The galaxy appears elongated, cigar-shaped in form, with a relatively high degree of central concentration. No distinct spiral arm structures or prominent dust lanes are discernible in this image. There are no indications of major ongoing mergers or significant tidal disturbances. Overall, the galaxy seems to be a relatively undisturbed system.
