The galaxy presents as a face-on spiral, exhibiting a prominent central bulge with a yellow-orange hue suggesting an older stellar population. Faint spiral arms extend outward, but they are not sharply defined. The color of the arms appears more bluish, potentially indicating more recent star formation activity. The spiral structure appears flocculent, with a somewhat irregular winding pattern. The galaxy shows no obvious signs of major disturbances or ongoing mergers, though the overall appearance suggests some gravitational interaction might have occurred.
