The galaxy appears to be relatively compact, with a concentrated central region exhibiting high luminosity. The core shows a bright, almost saturated appearance in the available imagery, indicating potentially intense activity, such as a supermassive black hole or a high rate of star formation. Surrounding the central core, a less luminous, extended halo is visible. This halo appears amorphous with what seems to be patchy areas, indicating a lack of defined spiral arms or a smooth, elliptical structure. There are some subtle color variations within the halo, showing a slight shift from green to purple near the bottom, possibly representing areas of varying stellar populations or dust content. These slight asymmetries may hint at tidal interactions or recent minor mergers. Overall, the galaxy appears relatively undisturbed with a bright, potentially active nucleus.
