The galaxy presents as a spiral, though the morphology is somewhat indistinct. The spiral arms appear tightly wound, tracing a path close to the central bulge. The bulge itself is prominent, exhibiting a bright, concentrated luminosity. The disk appears relatively smooth, with a moderate inclination relative to our line of sight. There is some evidence of a bar structure, most likely weak, though there are no obvious signs of interaction or disturbance of the overall spiral structure.
