The galaxy presents as a spiral with a relatively large bulge compared to the disk. While the galaxy is viewed close to face-on, the spiral arms are evident and show a structure that winds relatively tightly around the bulge. Two spiral arms are particularly visible. The bulge is a yellowish-white hue, suggesting an older stellar population. The disk appears bluish, indicative of ongoing star formation. There's no obvious bar structure bisecting the galaxy's central region. The galaxy does not appear to show any signs of ongoing or recent merger activity or major disturbances. The spiral arms show smooth and continuous arcs, suggesting a relatively undisturbed morphology.
