  WRA 751 is an evolved massive star in our Galaxy closely resembling Luminous
Blue Variable stars (LBVs). It is surrounded by a nitrogen enriched nebula of
ab out 23" diameter. A comparative study of the nebula's morphology and
kinematics is presented, it supports - together with spectroscopical evidence -
the classification of WRA 751 as a LBV. Images show that the nebula consists of
a nearly spherical shell as well as a bipolar-like structure north and south of
its main body, the Northern and Southern Caps. In contrast to the almost
spherical appearance of the main body of the nebula, the kinematics shows a
deviation even of this part from a classical spherical expansion pattern. From
the present data it can be concluded that the main body expands asymmetrically
(central expansion velocity ~26 km/s), with a thicker shell at the back side. A
bump-like structure can be found to the west of the central star. In addition
to the main body, bipolar kinematic components can be identified with the
morphologically classified Caps. These results put WRA 751 into the class of
LBVs which are surrounded by a nebula with bipolar components, albeit
considerably less pronounced than, for instance, in the classical bipolar LBVs
Eta Car and HR Car.
