This galaxy presents as a generally smooth, centrally concentrated object. It displays an elliptical morphology with a high degree of central light concentration. The color gradient transitions smoothly from a redder core to slightly bluer outer regions. The galaxy does not show any obvious spiral arm structures or prominent dust lanes, indicating a likely lack of significant ongoing star formation in the disk. There are some minor asymmetries or disturbances in the outer halo, that are likely caused by either minor interactions or internal processes. The galaxy appears relatively isolated, showing no immediate signs of major merging activity.
