The galaxy exhibits a smooth, elliptical morphology. It has a concentrated central bulge, surrounded by a more diffuse halo. The color gradient suggests a population of older stars in the outer regions, appearing redder, while the core region shows bluer hues, indicating the presence of younger stars or ongoing star formation. There is little evidence of spiral arms or significant dust lanes within the galaxy. The overall shape is somewhat elongated, with a minor axis to major axis ratio suggesting a moderate degree of flattening.
