The cosmology analyses of the Year-3 (Y3) data from the Dark Energy Survey (DES) is at full speed ahead. Our preliminary weak lensing sample contains 120 million objects over 4200 square degrees of sky and is the largest shape catalog to date. This statistical power comes at a price: the cosmic shear measurements are more sensitive not only to the signal but also to potential systematics. In this talk, I will present our prospects for the 2-point cosmic shear analysis and some of the leading systematics that must be under control, in particular the Intrinsic Alignments of galaxies. Additionally, I will talk about a novel detection of shear 3-point correlations in DES-Y3 simulations and data.