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A perturbative description of the Large Scale Structure (LSS) is a pillar of our understanding of the observed distribution of matter in the Universe. Renormalization is an essential and defining step to make this description physical and predictive. In this talk I will start by a concise review of the preliminaries of the standard perturbation theory (SPT) and diagrammatic representation of perturbation theory. Next I will try to elaborate the very meaning of "renormalization" in the Effective Field Theory of Large Scale Structure (EFT of LSS) and the structure of the so-called counter-terms. In closing I will show the results of the EFT of LSS approach are in a percent level agreement with the numerical data.