  We present the far-ultraviolet spectrum of the Seyfert 1 galaxy 2MASX
J21362313-6224008 obtained with the Far Ultraviolet Spectroscopic Explorer
(FUSE). The spectrum features absorption from Galactic OVI at two velocities
and redshifted HI Lyman beta and gamma, CII, CIII, and O VI. The redshifted
absorption features represent a single kinematic component blueshifted by ~310
km/s relative to the AGN. We use photoionization models to derive constraints
on the physical parameters of the absorbing gas. An alternative interpretation
for the absorption lines is also proposed, whereby the absorbing gas is
associated with an intervening galaxy cluster.
