The galaxy presents as an elliptical or lenticular system, appearing mostly smooth and featureless. It exhibits a centrally concentrated brightness profile, with a gradual decrease in luminosity extending outwards. The morphology suggests a relatively evolved system with a dominant bulge component. Color gradients are subtle, but hint at bluer hues in the outer regions and yellow hues in the center, possibly indicating differential stellar populations with ongoing star formation in the outer disk. The galaxy appears undisturbed, lacking prominent tidal features or signs of a recent major merger. The overall shape indicates a somewhat flattened ellipsoid, rather than a perfect sphere, suggesting some rotational support. There might be some minor distortions in its shape, but if they are present, they would be considered to be very minor and subtle. 
