The galaxy presents a disturbed morphology, potentially indicative of an ongoing or recent interaction. It exhibits an elongated shape with a distinct, brighter central region, possibly a bulge. A faint tidal tail extends away from the main body, suggesting gravitational disruption. The galaxy displays variations in color, with bluer regions possibly indicating areas of active star formation, and redder regions potentially representing older stellar populations or dust obscuration. The overall structure is complex, lacking the clear spiral arm structure of grand design galaxies, and appears rather amorphous. Patches of luminous material are distributed throughout, with an irregular distribution and varied brightness levels, pointing to a complex star formation history.
