The galaxy presents as an elliptical or lenticular type, characterized by a smooth, concentrated light profile without discernible spiral arms or a significant disk-like structure. The color appears generally yellowish-orange, suggesting an older stellar population with fewer young, hot stars, indicative of low current star formation. It is fairly round in shape, with no major distortions or tidal features visible, suggesting it is unlikely to be undergoing a major merger. The light appears quite concentrated in the center, and diffuses at its edges. The galaxy appears relatively undisturbed and isolated.