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In 2013, the IceCube Neutrino Observatory located at the geographic SouthPole detected evidence for a diffuse astrophysical neutrino flux above ~60 TeV.To this day, IceCube has operated with full detector configuration for morethan 6 years. The observed astrophysical neutrino flux has been confirmed with> 6$\sigma$ significance with both events starting within the detector (allflavor) and events traversing through the Earth ($\nu_{\mu}$ charged-current).Somewhat equal flavor ratio of astrophysical neutrinos is expected at Earthassuming standard thorough oscillation. A search for tau neutrinos has beencarried out but yielded null result. No neutrino sources have been found tocontribute significantly to the diffuse flux at this point. In this paper, wewill review the current status of the astrophysical neutrino flux, discuss thequest for neutrino point sources and overview the proposed design and physicspotentials of the future IceCube-Gen2.

Exploring the Universe with Neutrinos: Recent Results from IceCube