The galaxy exhibits a notable disk structure, though the orientation presents a near face-on view. Well-defined spiral arms are apparent, indicating ongoing or recent star formation. A bar-like structure appears to be present traversing the galactic center, possibly influencing the spiral arm morphology. The bulge component is discernable but not dominant, appearing to be of moderate size relative to the overall galactic structure. The galactic disk shows some signs of minor disturbances, the overall morphology remains relatively intact, suggesting no major merging events are currently in progress. The system displays a slightly blurred appearance, possibly indicative of its redshift.
