  We present optical and radio images, and long-slit spectra of the radio
galaxy PKS 1932-464 (z=0.230). Our main goal is to determine whether the
observed properties of the extended emission line nebulosity in this object
show evidence for interactions between the radio jet and the extended ionized
gas, or whether they can be explained in terms of the illumination of the
extended gas by the active nucleus. Although the data do not show compelling
evidence for jet-cloud interactions, the existence of two well distinguished
emitting line regions with very different kinematics and ionization levels
suggests the presence of such interactions. The large-scale gas distribution is
complex and suggests a gravitational interaction between the host galaxy of PKS
1932-464 and a nearby companiongalaxy. The detection of a broad Ha emission
line in the nuclear spectrum of the object provides evidence that this object
is a broad line radio galaxy (BLRG) rather than a narrow line radio galaxy
(NLRG) as previously supposed.
