The galaxy presents as a somewhat elliptical, smooth structure with a concentrated central bulge that exhibits a yellowish hue, possibly indicative of an older stellar population. A diffuse, bluer halo surrounds this central region, suggesting the presence of a younger stellar population. The overall morphology appears relatively undisturbed, with no obvious signs of ongoing major mergers or significant tidal interactions. Some very subtle features are visible in the outer regions, potentially indicative of a faint disk or arm structures. The axial ratio suggests it is not viewed face-on. The galaxy's color profile transitions smoothly from the yellow core to the bluer outer regions, possibly resulting from recent star formation.
