The galaxy presents a clear spiral structure, with prominent, well-defined arms. The arms appear somewhat flocculent, displaying a mix of medium to loosely wound patterns. Star forming regions are visible within the spiral arms.

The central bulge region exhibits a moderate size relative to the overall galactic disk. No strong bar feature is immediately apparent, but the possibility of a weak bar cannot be excluded based on visual inspection.

Evidence suggests the galaxy is experiencing some form of interaction or disturbance. The morphology seems to be distorted, potentially indicating tidal forces or a merger event. A notable disruption appears to be occurring.
