This galaxy exhibits a predominantly smooth morphology, showing a significant central bulge. The light distribution suggests a shape that is neither perfectly round nor highly elongated. There may be slight irregularities or distortions within the galaxy's structure, but the overall form appears relatively undisturbed.

Color gradients indicate varying stellar populations or dust content within the galaxy. The central region shows evidence of hotter, younger stars, while the outer regions appear to contain cooler, older populations.
