The galaxy presents a smooth, elliptical morphology. It exhibits a concentrated central bulge that appears spheroidal in shape, with a gradual decrease in luminosity moving outward. The color profile suggests a dominance of older stellar populations, with a yellowish-orange hue indicative of evolved stars. There is no discernible evidence of spiral arm structures or significant dust lanes. The galaxy does not appear to be undergoing any major mergers or tidal interactions with neighboring galaxies, with no apparent distortions in its overall shape. The smooth light distribution suggests it is an early-type galaxy that has largely ceased active star formation.
