The galaxy appears as a yellowish, elliptical-shaped object. It exhibits a relatively smooth light distribution without prominent spiral arms or dust lanes visible. The color suggests an older stellar population, with fewer young, hot stars. The galaxy does not show obvious signs of a recent major merger, although a minor disturbance cannot be ruled out based on this image alone. The morphology indicates that it is likely a lenticular or early-type spiral galaxy seen at a significant distance, contributing to its lack of discernible detailed structure. The round shape suggests it is not a highly inclined disk galaxy. Overall, the galaxy presents itself as a quiescent system dominated by evolved stars.
