The galaxy presents as a spiral type, exhibiting a distinct disk structure. The central bulge appears prominent and moderately sized, characterized by a smooth, concentrated light distribution, suggesting an older stellar population.

Spiral arms are readily discernible, displaying a morphology that could be classified as grand design. The arms are relatively tightly wound around the bulge, presenting a medium pitch angle. Evidence suggests two dominant spiral arms. The color gradient across the arms indicates ongoing star formation, with bluer hues observed in regions further from the galactic center.

The overall disk appears relatively undisturbed. The light distribution in the disk shows a moderate level of symmetry, and there is no immediately apparent indication of tidal features or significant morphological distortions. This suggests a relatively quiescent evolutionary history, free from major mergers or gravitational interactions in the recent past.
