The galaxy presents a morphology consistent with a spiral galaxy, exhibiting prominent spiral arms. These arms appear relatively tightly wound around a central bulge. The bulge seems of moderate size relative to the galactic disk. The galaxy appears face-on, providing a clear view of its spiral structure. There is some indication of flocculent spiral arm structure. No strong bar feature is immediately apparent. Evidence suggests it is not currently undergoing a major merger event, though minor tidal disturbances cannot be ruled out based on the image alone. The overall color suggests active star formation within the galaxy.
