We investigate the renormalization structure of scalar Galileons in flat spacetime. We explicitly calculate the ultraviolet divergent one-loop contributions to the 2−point, 3−point, 4−point, and 5−point functions. We discuss the structure of the counterterms and their hierarchy within an effective field theory expansion. We comment on different resummation schemes, including a geometric resummation for which our results could be generalized to arbitrary n−point functions.Keywords: modified gravity, physcis of the early universe, effective field theory, quantum field theory in curved spacetime, renormalization arXiv:1909.04662v1 [hep-th]