The galaxy presents as a spiral type, characterized by a prominent disk structure. The spiral arms are loosely wound, displaying a somewhat flocculent morphology. Two major spiral arms are discernible, although other fainter arms may be present. The central bulge is of moderate size, with no clear signs of a dominant spheroidal component. The disk is viewed at an angle close to face-on. A bar structure appears present across the galaxy's nucleus, but is not particularly strong. The spiral arms exhibit variations in color, potentially indicating varying stellar populations and active star formation regions. There seems to be some morphological disturbance, possibly suggestive of minor interactions with other galaxies.
