The galaxy presents as a spiral galaxy, seen at an oblique angle, but not quite edge-on. The galactic disk shows distinct spiral arm structure with a clear, organized pattern. The spiral arms exhibit loose winding. The image suggests the presence of two dominant spiral arms, emanating from the central region.

A prominent central bulge is observed. The bulge appears yellow and has a smooth texture, indicating an older stellar population. The bar structure of the galaxy appears to be weak.

There is limited evidence of a major ongoing merger. There is very little sign of disturbance in the morphology.

The stellar population appears older in the center and appears to be more actively forming stars in the arms.
