The galaxy presents as a spiral type, exhibiting a well-defined disk structure and prominent spiral arms. These arms appear tightly wound around a central bulge. The bluer hues observed in the spiral arms likely indicate regions of ongoing star formation, while the yellowish-white color of the bulge may indicate an older stellar population. The galaxy displays a relatively high degree of symmetry, with a smooth decline in light intensity from the center outwards. Faint traces of what appears to be a bar are visible in the central region, but it appears to be relatively weak. There are no indications of major disturbances or merger events in the overall morphology. The orientation of the galaxy allows for a clear view of the disk, as it does not appear to be edge-on. Overall, this galaxy seems to be a relatively undisturbed spiral galaxy with ongoing star formation concentrated in its arms.
