  We present MeerKAT L-band (886-1682 MHz) observations of the extended radio
structure of the peculiar galaxy pair PKS 2130-538 known as the "Dancing
Ghosts". The complex of bending and possibly interacting jets and lobes
originate from two Active Galactic Nuclei hosts in the Abell 3785 galaxy
cluster, one of which is the brightest cluster galaxy. The radio properties of
the PKS 2130-538 flux density, spectral index and polarization - are typical
for large, bent-tail galaxies. We also investigate a number of thin extended
low surface brightness filaments originating from the lobes. Southeast from the
Dancing Ghosts, we detect a region of low surface brightness emission that has
no clear origin. While it could originate from the Abell 3785 radio halo, we
investigate the possibility that it is a radio relic or emission associated
with the two PKS 2130-538 hosts. We find no evidence of interaction between the
two PKS 2130-538 hosts.
