The galaxy presents a largely smooth, elliptical morphology. A bright, concentrated central bulge dominates the overall structure, exhibiting a yellowish-white hue indicative of an older stellar population. The outer regions display a more diffuse, bluish halo, possibly indicating regions of more recent, though subdued, star formation. There is some indication of very faint disk-like structure. There is little to no evidence of spiral arms or significant dust lanes. A minor asymmetry or faint feature is barely present. There are no apparent signs of major mergers or significant tidal disturbances in its immediate vicinity. Overall, it appears to be a relatively undisturbed system.
