  We investigate the velocity distribution of elliptical galaxies in the
framework of Non-local Gravity. According to this approach, it is possible to
recover the fundamental plane of elliptical galaxies without the dark matter
hypothesis. Specifically, we compare theoretical predictions for circular
velocity in Non-local Gravity context with the corresponding values coming from
a large sample of observed elliptical galaxies. We adopt the surface
brightness, effective radius and velocity dispersion as structural parameters
for the fundamental plane. As final result, it is possible to show that
non-local gravity effects can reproduce the stellar dynamics in elliptical
galaxies and fit consistently observational data.
