The galaxy presents as a spiral type, observed at an oblique angle. The disk exhibits distinct spiral arm structures, appearing somewhat loosely wound. Two prominent arms are discernable. A central bar is suspected, bisecting the galaxy's core region. The bulge is relatively small or non-existent. The galaxy appears to be undergoing significant star formation, as indicated by its blue color. Some disturbances are visible, implying that the galaxy is undergoing a minor or major disturbance. Overall, this is a spiral galaxy with two arms, potentially with a central bar, an indistinct bulge, loose spiral arms, and hints of an ongoing merger.
