The galaxy presents as a face-on spiral structure. It exhibits tightly wound spiral arms, predominantly showing a two-arm configuration. The central bulge is relatively small and faint, with a yellow/white hue, suggesting an older stellar population. The spiral arms display a bluish tint indicative of ongoing star formation. There is no sign of any disturbance to suggest that the galaxy is in a major merger event. Weak evidence of a bar structure is apparent, though not distinctly pronounced. There is no sign of a prominent bulge, or a bulge at all.