The galaxy presents as a face-on spiral system. A prominent central bulge is visible, exhibiting a yellow-white hue, indicative of an older stellar population. The disk component shows a somewhat flocculent spiral arm structure. Several spiral arms can be traced, exhibiting a moderate winding. Some arms appear more tightly wound. The disk has a blue tinge, indicative of younger stars and ongoing star formation. There is an absence of a strong bar structure across the central region. The galaxy shows no signs of a major merger event, though a minor disturbance may be present within the disk structure. 
