The galaxy appears to be a relatively smooth, elliptical or lenticular system. It exhibits a centrally concentrated bulge that dominates its overall structure. The galaxy displays a slight elongation, with a ratio of minor to major axis of approximately 0.7 to 0.8, indicating it is not perfectly spherical. There's a subtle color gradient, with the central region appearing more yellow/orange, suggesting an older stellar population, while the outer regions show a slightly bluer hue, which could indicate the presence of some younger stars or ongoing, but limited, star formation. There are no prominent spiral arms or distinct dust lanes visible in this image. The outer edges fade gradually into the background, suggesting a smooth decline in stellar density. Overall, the galaxy presents a fairly regular and undisturbed morphology.
