The galaxy presents an overall elliptical morphology, appearing largely smooth and concentrated towards its center. There is a slight elongation visible, deviating from a perfectly circular shape. The galaxy exhibits a color gradient, transitioning from a more yellow/red hue at the core to a slightly bluer tinge in the outer regions, which may indicate subtle differences in stellar populations or dust content. There is some indication of potential tidal disturbances, although the overall appearance is relatively undisturbed. While the bulk of the galaxy appears consistent with an elliptical structure, the subtle color variations, slight disturbances, and elongation suggest a complex evolutionary history, possibly involving minor interactions or past mergers. The galaxy is relatively compact.
