The galaxy presents as an elliptical-like structure, though not perfectly spherical. There is a bright central bulge which appears relatively smooth and concentrated, indicating a possible supermassive black hole at the center. The outer regions show some irregularity, suggesting a degree of disruption. There are hints of a disk component, possibly containing spiral arms, though this is not definitively observed in this image. There is evidence of active star formation, as indicated by bluer hues scattered throughout the galactic body, particularly within the disk-like structure. Some distortions and tidal features indicate it is potentially undergoing, or has recently undergone, a merger or interaction with another galaxy, resulting in the observed asymmetry. Overall, the galaxy appears as a complex system with a combination of old stellar populations in the central bulge and newer star formation in its disk.
