The galaxy presents a distinct spiral morphology. Two prominent spiral arms emanate from a central region. These arms appear loosely wound. The bulge is relatively small and indistinct. A subtle bar-like structure seems to be present across the bulge. The disk is the dominant feature, with spiral arms that appear to be actively forming stars, based on their bluish tint. The overall shape suggests minimal signs of recent major merger events, though some slight distortion in the arms could indicate minor interactions.
