The galaxy presents as a spiral type, exhibiting a disk-like structure with discernible spiral arms. The winding of the spiral arms appears to be relatively tight.

The central bulge is relatively small and not dominant.

There are disturbances and possible merging visible, and these are likely playing a role in the current morphology of the system.

The galaxy displays a color gradient, with the central regions appearing more yellowish, potentially indicating an older stellar population. The spiral arms exhibit a bluer hue, which could be indicative of ongoing or recent star formation.
