The galaxy presents a somewhat elliptical morphology, appearing moderately smooth in texture with some indication of disk-like features. The central region displays a higher surface brightness and a slightly yellow hue. The outer regions appear fainter with a bluer color, perhaps indicative of ongoing star formation in these areas. There's a hint of disturbance or asymmetry in the galaxy's structure, though it doesn't appear to be undergoing a major merger. The overall light distribution suggests that the galaxy is dominated by an intermediate-aged stellar population, with a possible contribution from younger stars in the outer arms. The relative smoothness implies the system is relatively evolved, but the bluer color and slight disturbances may suggest recent or ongoing accretion events or minor mergers.
