  We consider Galileon inflation in the Effective Field Theory (EFT) framework
and examine the possibility for PBH formation during slow roll (SR) to ultra
slow roll (USR) transitions. We show that loop corrections to the power
spectrum, in this case, do not impose additional constraints on the masses of
PBHs produced. We indicate that the remarkable non-renormalization property of
Galileans due to generalized shift symmetry dubbed as Galilean symmetry is
responsible for protecting PBH formation from quantum loop corrections.
