The galaxy appears to be a spiral galaxy, displaying a significant disk component. The disk is oriented at an angle relative to our line of sight, presenting an oblique view. Two distinct spiral arms are readily apparent. There appears to be moderate winding in the spiral arms. 

A central bulge is present. The size of the bulge is moderate relative to the size of the galaxy's disk. A subtle bar-like structure is also discernible across the central region. No interactions or tidal features are obvious in the galaxy's morphology. The appearance of merging is not apparent, displaying a seemingly undisturbed morphology.
