verify that there are stars detected everywhere in the image in the ‘Dynamic PSF’ window and adjust parameters if it’s not the case
change the limit magnitude slightly, depending on how many stars are found.
change the used catalogue, sometimes that helps too
use an external plate solver like astrometry.net (the local version works from Siril) or ASTAP (calling it manually) then use Siril to run the PCC on the solved image
Solving wide field images is always tricky because of the distorsion and the fact that it’s harder to distinguish stars that are very near from each other in the image.