This appears to be a spiral galaxy, viewed at an angle intermediate between face-on and edge-on. The galaxy exhibits a central bulge region that is relatively bright and concentrated. The disk shows distinct spiral arm structures. These arms are wound tightly around the bulge, indicating possibly strong shear forces from galactic rotation. The disk appears to have a relatively high concentration of star formation. Although, the bulge is smooth without any features. The spiral arms exhibit a clumpy morphology, suggesting active regions of star formation within them. No significant tidal distortions or signs of major mergers are immediately apparent in the morphology. It's difficult to determine the exact number of spiral arms due to the imaging resolution and orientation, but there is possible evidence of three or four arms.
