  The Telescope Array (TA) is an experiment to observe Ultra-High Energy Cosmic
Rays (UHECRs). TA's recent results, the energy spectrum and anisotropy based on
the 6-year surface array data, and the primary composition obtained from the
shower maximum Xmax are reported. The spectrum demonstrates a clear dip and
cutoff. The shape of the spectrum is well described by the energy loss of
extra-galactic protons interacting with the cosmic microwave background (CMB).
Above the cutoff, a medium-scale (20 degrees radius) flux enhancement was
observed near the Ursa-Major. A chance probability of creating this hotspot
from the isotropic flux is 4.0 sigma. The measured Xmax is consistent with the
primary being proton or light nuclei for energies 10^18.2 eV - 10^19.2 eV.
