The galaxy presents as a spiral type, though somewhat irregular. A central bulge is discernible, appearing relatively small compared to the disk. The spiral arms are prominent and exhibit a flocculent structure, with regions of active star formation visible as localized bright spots. The arm winding appears moderate in tightness. There is no obvious strong bar structure. The galaxy is viewed nearly face-on, precluding observations of a distinct edge. The overall morphology suggests ongoing or recent star formation activity within the disk. The galaxy shows no obvious signs of major interaction or mergers but some disturbances are visible.
