  We present a high spatial and spectral resolution 2-D echelle spectrogram of
the Narrow-Line Region in the Seyfert 2 galaxy NGC1386. This Seyfert galaxy was
observed with CASPEC in the wavelength range 5270-7725 Angstrom which covers
the H-alpha and the [N II] lines. With the use of spatially high resolved
images taken with the WFPC2 aboard the Hubble Space Telescope we could identify
individual components of the Narrow-Line Region in our spectra. A Gaussian
decomposition of the spectra revealed 9 distinct emission-line complexes. The
brightest component is blue-shifted by -120+-10 km/s with respect to the
systemic velocity and shows an offset of -1.6" relative to the nucleus of the
galaxy. The true nucleus of NGC1386 has a much lower apparent H-alpha
luminosity than this component. The nucleus is probably highly absorbed.
Although the majority of the Narrow-Line Region components follows a regular
velocity field, we find evidence for a separate kinematic component. The
Narrow-Line Region is aligned anti-parallel to the radio-jet which propagates
from the center of NGC1386 to the south.
