We present high resolution images in the photometric bands V, R, I, J,
H and K of a remarkable bipolar nebula we named the ''Flying Ghost Ne
bula'' (FGN) from both its optical shape and its lack of detection by
the IRAS satellite. We interpret these images in term of a central you
ng bright star of intermediate mass surrounded by a circumstellar disk
seen almost perfectly edge-on. We find that the central object is a 4
M. B star and the size and mass of its circumstellar disk are respect
ively of the order of 1500 AU and 0.03 M. The Flying Ghost Nebula coul
d be a rare example of an intermediate mass star formed from a flatten
ed structure not yet dissipated.