The galaxy presents a distinct spiral morphology, viewed approximately face-on. A central bulge is discernible, appearing relatively small in proportion to the disk. Two prominent spiral arms emanate from the central region and appear to wrap around the disk, displaying a medium winding. No strong bar structure is evident. The color gradient suggests younger stellar populations reside within the spiral arms, indicated by the bluer hues, while the bulge exhibits a yellower, potentially indicative of an older stellar population. There is no sign of major mergers, but the disk could be slightly disturbed.
