The galaxy exhibits a clear spiral structure. Two distinct spiral arms are visible emanating from a central bulge. The bulge appears relatively moderate in size compared to the overall disk. The winding of the spiral arms seems to be somewhere between medium and loose. The galaxy displays a central bar feature spanning across the bulge. The bar has fairly strong presence. There is evidence of ongoing merger activity or significant gravitational disturbance, potentially influencing the overall morphology of the galaxy. The disk of the galaxy is not oriented edge-on.
