The galaxy presents as an elliptical morphology. It displays a largely smooth structure, with a highly concentrated central bulge. The color gradient transitions from a yellowish core to a subtly bluer outer halo. No distinct spiral arm structures or bar features are apparent within the visible portion of the galaxy. There is little to no indication of active star formation regions, which is consistent with an older stellar population. The galaxy exhibits a high degree of roundness, with no major distortions suggesting recent or ongoing merger activity. Faint extensions or tidal features are not visible, suggesting relative isolation.
