The galaxy presents as a largely featureless elliptical type with a concentrated central bulge. The light distribution exhibits a smooth gradient, transitioning from a bright, dense core region outward to a more diffuse halo. There appears to be a slight elongation along one axis, deviating marginally from a perfectly circular form. Color gradients are subtle, with the core showing a yellowish hue potentially indicating an older stellar population, while the outer regions are fainter with hints of blue, which could suggest trace amounts of more recent star formation. The morphology suggests a system that has largely completed its major mergers and is in a relatively quiescent state. There's no discernible evidence of tidal features or strong gravitational disturbances, and there are no clear indications of active star formation regions.