  We derive gravitational waves in a theory with non-local curvature
corrections to the Hilbert-Einstein Lagrangian. In addition to the standard two
massless tensor modes, with plus and cross polarizations, helicity 2 and
angular frequency $\omega_{1}$, we obtain a further scalar massive mode with
helicity 0 and angular frequency $\omega_{2}$, whose polarization is
transverse. It is a breathing mode, which, at the lowest order of an effective
parameter $\gamma$, presents a speed difference between nearly null and null
plane waves. Finally, the quasi-Lorentz $E(2)$-invariant class for the
non-local gravity is type $N_{3}$, according to the Petrov classification. This
means that the presence (or absence) of gravitational wave modes is
observer-independent.
