The galaxy presents as a barred spiral, with a prominent central bulge. The bar structure appears to extend through the core region, affecting the morphology of the inner arms. Two spiral arms are clearly visible, one on either side of the central bulge. These arms exhibit a medium winding, and are not tightly wound around the central bulge. The disk is oriented nearly face-on. There is evidence of active star formation within the spiral arms. There may be some minor disturbance in its structure, but it is largely intact.
