  The Seyfert 2 galaxy NGC 2110 has been observed with BeppoSAX between 0.5 and
150 keV. The high energy instrument onboard, PDS, has succeeded in measuring
for the first time the spectrum of this source in the 13-150 keV range. The PDS
spectrum, having a photon index Gamma~1.86 is fully compatible with that
expected from a Seyfert 1 nucleus. In the framework of unified models, the
harder (Gamma~1.67) 2-10 keV spectrum is well explained assuming the presence
of a complex partial + total absorber (Nh~30x10^22 cm^-2 x25% + Nh~4x10^22
cm^-2 x100%). The high column density of this complex absorber is consistent
both with the FeK_alpha line strength and with the detection of an absorption
edge at E~7.1 keV in the power-law spectrum.
