  We present radio observations of the radio galaxy PKS 2152-699 obtained with
the Australia Telescope Compact Array (ATCA). The much higher resolution and
s/n of the new radio maps reveals the presence of a bright radio component
about 10 arcsec NE of the nucleus. This lies close to the highly ionized cloud
previously studied in the optical and here shown in a broadband red snapshot
image with the HST PC2. It suggests that PKS 2152-699 may be a jet/cloud
interaction similar to 3C277.3. This could cause the change in the position
angle (of ~20 deg) of the radio emission from the inner to the outer regions.
On the large scale, the source has Fanaroff & Riley type II morphology although
the presence of the two hot-spots in the centres of the lobes is unusual. The
northern lobe shows a particularly relaxed structure while the southern one has
an edge-brightened, arc-like structure.
