The galaxy appears to be a spiral galaxy exhibiting prominent spiral arm structures. The arms are loosely wound and are composed of a clumpy distribution of stars and gas. There is a slight indication of having two or more spiral arms. The central bulge appears relatively small to moderate in size, showing a brighter, more concentrated region of light suggesting an older stellar population. The disk is viewed at an angle, but does not seem to be fully edge-on. There are no visible signs of a strong bar structure bisecting the bulge. There are some minor disturbances, but the galaxy appears to be relatively undisturbed in its overall morphology. The galaxy exhibits a blue hue in its arms, which is associated with ongoing star formation.
