  We report the discovery of a z=2.76 radio galaxy, MG1019+0535, with an
unusual spectrum. Ly$\alpha$, which usually dominates the spectra of high
redshift radio galaxies, is very weak and the strongest lines in the spectrum
are CIV$\lambda$1549 and HeII$\lambda$1640. We speculate that dust is
responsible for attenuating the Ly$\alpha$ line. This object provides more
evidence for dust formation at early epochs. The optical counterpart of the
compact radio source has a double morphology which is orthogonal to the radio
source axis and most likely due to the superposition of two distinct objects
which may or may not be physically related. There is only one detected line
from the brighter component (B) which is close in observed wavelength to the
redshifted HeII$\lambda$1640 line from the z=2.76 galaxy (A). We discuss
whether B is at the same redshift as A or whether it is a foreground galaxy at
z=0.66. We also report the serendipitous discovery of a very red ($R-K>7$)
field object.
