The observed galaxy presents as a spiral galaxy, viewed at a relatively high inclination. The morphological structure is dominated by a prominent disk, displaying well-defined spiral arms. These arms exhibit a tightly wound morphology, suggesting differential rotation and gravitational interactions within the galactic structure. It is difficult to discern the exact number of spiral arms as the galaxy is highly inclined, with half of its arms obstructed from our view. The spiral structure shows a degree of patchiness, potentially indicating regions of active star formation. The central bulge appears to be of moderate size. No obvious bar structure is apparent. There is no clear evidence of a major ongoing merger, although minor disturbances cannot be ruled out. The general color profile suggests a moderately actively star-forming galaxy.
