Neutrino oscillation experiments, both ongoing and upcoming, alongside their synergies, lay the cornerstone for resolving key issues within the framework of the three-flavor neutrino paradigm. The present complementarities between atmospheric and long-baseline experiments have reduced the span in atmospheric oscillation parameters and the CP phase. Further, the persistent discrepancy between Solar and KamLAND data regarding $\Delta m^2_{21}$ has now been almost resolved. The remarkable precision on $\theta_{13}$ attained by the current reactor experiment, Daya Bay is unprecedented. The notable precision attained in ongoing oscillation experiments not only lays a solid foundation for future research but also offers the potential for substantial advancements and the revelation of significant phenomena within the neutrino sector. This work briefly highlights the recent advancements and outlines the promising future directions in the field of neutrino oscillations.