The galaxy appears to be an elliptical galaxy, exhibiting a smooth, generally featureless morphology. There is a bright central bulge that fades gradually outwards. Its shape is moderately round. There is no prominent disk structure observed, and there is no significant sign of merging activity or major disturbances. Color gradients are subtle; the central region presents slightly bluer hues compared to the faint, extended outer regions which appear more red. This could indicate older stellar populations in the outer halo. There is no indication of recent star formation.