  We report spectroscopic observations of the nova M31N-2007-06b, which was
found to be spatially coincident with the M31 globular cluster Bol 111. This
nova is the first out of more than 700 discovered in M31 over the past century
to be associated with one of the galaxy's globular clusters. A total of three
spectra of the nova were obtained 3, 6, and 36 days post discovery. The data
reveal broad (FWHM ~3000 km/s) Balmer, NII, and NIII emission lines, and show
that the nova belongs to the He/N spectroscopic class. The He/N class of novae
are relatively rare, making up roughly 15% of the novae with measured spectra
in M31, and roughly 20-25% of the Galactic novae for which spectroscopic data
are available. The implications of a nova, particularly an He/N nova, occurring
in a globular cluster are discussed.
