The galaxy presents as a spiral type, displaying a prominent, tightly wound spiral arm structure. Multiple arms emanate from a central bulge region. The arms exhibit a clumpy morphology characterized by regions of intense blue emission, suggestive of active star formation. The central bulge appears relatively small and indistinct. The galaxy disk is viewed at a near face-on angle. There is a faint bar-like structure in the galaxy. The galaxy shows signs of minor tidal disruption and has not merged with any other large objects. The disk is fairly smooth.
