  We present scanning Fabry-Perot interferometric observations of CIG 993, an
apparently isolated luminous infrared galaxy also exhibiting luminous blue
compact and Wolf-Rayet galaxy features, as well as high star formation rate.
Our high resolution observations of the H$\alpha$ emission line allowed us to
derive the radial velocity field, as well as the velocity dispersion $\sigma$,
and the residual velocity fields of the galaxy. This galaxy exhibits several
kinematical components. On one hand, the velocity gradients detected on the
velocity field can be associated with a rotating disk -contrary to previous
results with less spectral resolution-. However, the velocity field, the
$\sigma$ and residual velocity field show significant deviations from circular
motions in the central part of the galaxy that matches a region with high
number of Wolf-Rayet and O stars, coincident with the blue luminous component
of the galaxy. We find narrow and broad velocity components for the ionized gas
in the central part of the galaxy. The broad component is evidence of a central
outflow related with the on-going burst of stellar formation. The
morpho-kinematical analysis of the galaxy indicates we are only seeing the
brightest parts of the galaxy which correspond to the bulge, a central bar and
the beginning of the disk. We believe CIG 993 is a disk galaxy harboring
important star-forming processes most likely caused by a relatively recent
interaction. This could imply that small encounters could change the global
characteristics of a galaxy without disturbing the main rotation disk motion,
nor the morphology of the galaxy.
