  We present spectral analysis of two Suzaku observations of the Seyfert 2
galaxy, NGC 2110. This source has been known to show complex, variable
absorption which we study in depth by analyzing these two observations set
seven years apart and by comparing to previously analyzed observations with the
XMM-Newton and Chandra observatories. We find that there is a relatively
stable, full-covering absorber with a column density of ~3$\times 10 ^{22}$
cm$^{-2}$, with an additional patchy absorber that is likely variable in both
column density and covering fraction over timescales of years, consistent with
clouds in a patchy torus or in the broad line region. We model a soft emission
line complex, likely arising from ionized plasma and consistent with previous
studies. We find no evidence for reflection from an accretion disk in this
source with no contribution from relativistically broadened Fe Ka line emission
nor from a Compton reflection hump.
