The galaxy presents a smooth, elliptical morphology with a noticeable central bulge. Its color profile exhibits a yellowish-white hue, indicative of an older stellar population, particularly within the bulge. Fainter, bluer regions are subtly dispersed throughout the galaxy and there are very slight hints of a possible disk. There's no apparent spiral arm structure or significant dust lane obscuration. The overall structure appears largely undisturbed, showing no obvious signs of recent major merger activity. Subtle irregularities and minor disturbances may be present, possibly due to minor interactions or internal processes, but the galaxy is predominantly smooth.