The galaxy appears as a centrally concentrated, roughly elliptical or lenticular system. The light profile decreases gradually from the center outwards, suggesting a smooth stellar distribution. There is no strong evidence of spiral arms or significant dust lanes within the galaxy. The overall color appears relatively uniform across the galaxy, indicating a lack of strong ongoing star formation. The galaxy exhibits a subtle bluish tint in its central region, suggesting the presence of a somewhat younger stellar population there as compared to its outer regions. The lack of apparent morphological disturbance implies that it has likely not undergone a recent major merger event. Based on its smooth appearance, it may be characterized as an early-type galaxy.
