The galaxy appears to be a relatively smooth, elliptical-type galaxy. Its overall color is yellowish-white, concentrated centrally, suggesting an older stellar population. The galaxy exhibits a slightly elongated shape, more like a disc, indicating a minimal degree of rotational support. The lack of distinct spiral arms or prominent dust lanes points to a system that has largely exhausted its gas supply and has a low star formation rate. There are no signs of merging or major disturbances in its morphology, suggesting it is a relatively isolated and stable system.
