  We present a datacube covering the central 10 arcsec of the archetypal active
galaxy NGC 1068 over a wavelength range 4200 to 5400 Angstrom. obtained during
the commissioning of the integral field unit (IFU) of the Gemini Multiobject
Spectrograph (GMOS) installed on the Gemini-North telescope. The datacube shows
a complex emission line morphology in the [OIII] doublet and Hbeta line. To
describe this structure phenomenologically we construct an atlas of velocity
components derived from multiple Gaussian component fits to the emission lines.
The atlas contains many features which cannot be readily associated with
distinct physical structures. While some components are likely to be associated
with the expected biconical outflow, others are suggestive of high velocity
flows or disk-like structures. As a first step towards interpretation, we seek
to identify the stellar disk using kinematical maps derived from the Mgb
absorption line feature at 5170 Angstrom and make associations between this and
gaseous components in the atlas of emission line components.
