In this talk, I’ll introduce the recent progress on the discrepancy between the measurements of the galaxy-galaxy clustering and lensing. As found by the recent literature, the current best-fitting models to the galaxy clustering measurements overestimate the corresponding galaxy-galaxy lensing measurements by 20%-40% at various scales, which raises a severe problem in using the clustering and lensing measurements to constrain the cosmology. In our recent works, we further investigate this problem by using the most recent measurements and confirm the previous conclusions.