The galaxy presents as a concentrated, elliptical form. Its central region exhibits a bright, yellowish-orange hue, suggesting a substantial population of older stars. The intensity gradually diminishes outwards, forming a relatively smooth, diffuse halo. There is no observable evidence of spiral arms or significant dust lanes, further supporting its classification as an elliptical galaxy. The overall morphology indicates a system that is likely evolved, with a relatively low rate of star formation, and no signs of major mergers or tidal disturbances.
