  We present a measurement of the cosmic-ray electron+positron spectrum between
7 GeV and 2 TeV performed with almost seven years of data collected with the
Fermi Large Area Telescope. We find that the spectrum is well fit by a broken
power law with a break energy at about 50 GeV. Above 50 GeV, the spectrum is
well described by a single power law with a spectral index of $3.07 \pm 0.02 \;
(\text{stat+syst}) \pm 0.04 \; (\text{energy measurement})$. An exponential
cutoff lower than 1.8 TeV is excluded at 95\% CL.
