We present photometric and spectroscopic observations of the late afterglow
of GRB 000911, starting similar to1 day after the burst event and lasting
similar to8 weeks. We detect a moderately significant re-brightening in the
R, I and J lightcurves, associated with a sizable reddening of the spectru
m. This can be explained through the presence of an underlying supernova, o
utshining the afterglow similar to 30 days after the burst event. Alternati
ve explanations are discussed.