  26W20, a radio galaxy located at a projected distance of 2.2 Mpc from the
center of Abell 754 (z=0.054) exhibits core emission properties similar to
those of a BL Lac object. New radio observations and VLA archival data show
parsec scale features in the core (L_{r} approx.10^{41}) ergs/s with a flat
spectrum. From observations with ROSAT, we demonstrate that the X-ray core
emission (L_{x}=3X10^{43}) ergs/s is non-thermal and variable. An 18% increase
in the X-ray luminosity was observed in two observations separated by five
days. The optical morphology is that of a large, normal elliptical galaxy
(m_{v}=15.6) and the optical spectrum lacks strong emission lines. If the
innermost segment of the radio jet is close to our line of sight, Doppler
boosting could explain both the observed X-ray intensity and the absence of
emitting line regions.
