The galaxy presents as a largely smooth, elliptical object. It has a centrally concentrated, bright core that gradually diffuses outward. The color profile suggests an older stellar population, with a yellowish-orange hue dominating the central region, fading into slightly bluer tones in the outer regions, hinting at some recent, though minimal, star formation. The overall shape is generally round, with no immediately apparent signs of spiral arms or a disk-like structure. There are no obvious indications of a major merger event. Close inspection reveals a subtle disturbance or minor asymmetry, though it is not significant enough to classify it as a major interaction. The light distribution is quite regular and lacks any prominent knots or irregularities in its outer isophotes.
