The next-generation survey observations for cosmological studies, such as Rubin and Euclid, are expected to start observation this year. To reveal the mystery of dark energy and dark matter in the Universe, these surveys will bring us unprecedented constraining power on cosmological parameters and ample opportunities to test beyond the standard cosmological model (LCDM). To understand where we are standing with the most recent observations, in my talk, I will overview the weak lensing analysis results of current surveys as well as the challenges, including the baryonic feedback effect. As a main builder of the Kilo-Degree Survey (KiDS), the current European Survey team, I will also introduce upcoming updates on the last release of the KiDS (KiDS Legacy) data, whose scientific results are scheduled to be announced this Autumn.