Modern precision cosmology is undergoing rapid development thanks to the measurements obtained from various types of the large scale cosmological surveys. In this talk, I will present the recently released DES-Y3 cosmological analysis results on the galaxy clustering and weak lensing measurements. Specifically, I will discuss the effect of baryonic feedback in the weak lensing analysis, and the implications of the current curiosities (or tensions) between different probes on some of the beyond-LCDM cosmological models.