The galaxy presents as a spiral galaxy, viewed at an oblique angle. Two prominent spiral arms are visible, winding outwards from a central bulge. The spiral arms are not tightly wound. The northern arm appears more diffuse and less defined than the southern arm.

A bar structure is present, oriented roughly horizontally through the central bulge. The bulge itself appears moderate in size. There is no obvious indication of a major merger event; however, there may be minor disturbances present in the morphology of the arms, potentially hinting at past interaction or ongoing accretion.
