  We present the results of our photometric and spectroscopic observations of
Nova Sco 2007 N.1 (V1280 Sco). The photometric data was represented by a single
data point in the light curve since the observation was carried out only for
one night. The spectra cover two different phases of the object's evolution
during the outburst, i.e. pre-maximum and post-maximum. Measurements of the
P-Cygni profile on Na I 'D' line (5889 \AA) was derived as the velocity of
shell expansion, yielding $1567.43 \pm 174.14$ km s$^{-1}$. We conclude that
V1280 Sco is a fast Fe II-type nova.
