The galaxy presents a generally smooth, elliptical morphology. Its core exhibits a bright, concentrated luminosity, appearing nearly spherical. Moving outward from the core, there is a gradual decrease in surface brightness. Faint hints of a disk-like structure are suggested by subtle color variations, although the dominant characteristic remains spheroidal. The color profile indicates the presence of both older stellar populations, represented by warmer tones, and some regions with bluer hues, potentially indicative of more recent star formation, albeit at a low rate. The overall structure appears undisturbed, showing no signs of major mergers or significant tidal interactions.
