The galaxy presents as an elliptical or lenticular type. The central bulge exhibits a bright, concentrated luminosity, suggesting a high density of stars. The overall form is smooth and relatively featureless, with a somewhat flattened shape. The galaxy demonstrates a color gradient, transitioning from a bluish-white hue in the central region to a yellowish-red tint in the outer regions, suggesting a population shift from younger, hotter stars in the core to older, cooler stars in the periphery. There appears to be little evidence of distinct spiral arms or significant dust lanes. The galaxy exhibits no signs of major tidal disturbances or ongoing mergers. The smooth, slightly elongated morphology suggests a system that has largely settled into a stable configuration.
