The galaxy presents as a spiral structure, with discernible spiral arms extending from a central bulge. The arms appear somewhat flocculent, exhibiting a patchy distribution of star formation. The bulge is moderately sized, not dominating the overall structure, but also not insignificant. There appears to be some disturbance to the morphology, which might be indicative of minor interactions. There is no clear evidence of a strong bar feature. The disk is observed close to face-on, allowing for a relatively clear view of the spiral structure.
