The galaxy presents as a spiral galaxy viewed at an oblique angle, slightly inclined from an edge-on perspective. Its disk structure is prominent, exhibiting a swirling pattern, although the exact number of spiral arms is difficult to discern. The spiral arms appear tightly wound and are somewhat fuzzy in appearance.

The galaxy possesses a central bulge which is relatively small compared to the overall size of the disk. The bulge exhibits a smooth texture.

There is no obvious presence of a strong bar structure transecting the bulge. The galaxy appears to be relatively undisturbed, showing no significant signs of an ongoing major merger event, although a possible minor disturbance is suggested by some asymmetry within the spiral arms. The color of the galaxy is consistent with the light emitted from aging stars.
