The observed galaxy presents as a relatively large spiral system. The morphology is that of a disk galaxy viewed at an oblique angle, but not quite edge-on. Distinct spiral arm structures are evident, appearing loosely wound. These arms exhibit a clumpy texture suggestive of active star-forming regions. The colour of the spiral arms seems to be bluer than the central bulge, also suggesting active star formation, which would indicate a high number of relatively young, massive stars.

The central bulge appears to be relatively small and exhibits a yellowish-white hue, indicating an older stellar population compared to the arms. There is little sign of a strong bar structure running through the center. Indications of merging or major disturbances are relatively low.
