The galaxy presents a clear spiral structure. The spiral arms appear well-defined and extend outward from a brighter central bulge. The central bulge is a prominent feature, exhibiting a relatively smooth and concentrated distribution of light.

The winding of the spiral arms is relatively tight. Multiple spiral arms are discernible. No clear evidence of a strong bar-like structure bisecting the central bulge is immediately apparent. The galaxy does not present any obvious signs of significant tidal distortions or ongoing major merger activity. There is no strong color variation apparent in the arms.
