The galaxy appears as a centrally concentrated, elliptical-like structure. It exhibits a smooth and largely featureless morphology, with the majority of its light emanating from a bright, diffuse core. This core transitions smoothly into the outer regions of the galaxy. There is a slight color gradient, with the central regions appearing more yellow and orange than the outer regions, which exhibit a more reddish hue. There is no evidence of spiral arms or a distinct disk component. The galaxy shows no signs of significant recent mergers or major disturbances, its overall structure appears relatively undisturbed. The galaxy appears to be relatively compact, with a defined edge and a relatively high concentration of stellar mass.
