  Giant radio relics are arc-like structures of diffuse, non-thermal
synchrotron radiation that trace shock waves induced by galaxy cluster mergers.
The particle (re-)acceleration mechanism producing such radio relics is
unclear. One major open question is whether relics can be formed directly from
a population of thermal seed electrons, or if pre-existing relativistic seed
electrons are required. In some cases AGN can provide such a population of
sub-GeV electrons. However, it is unclear how common this connection is. In
this paper we present LOFAR 140 MHz and VLA L-band radio observations, as well
as Chandra data of PSZ2 G096.88+24.18, a merging galaxy cluster system hosting
a pair of radio relics. A large patch of diffuse emission connects a bright
radio galaxy with one of the relics, likely affecting the properties of the
relic. We find that the most plausible explanation for the connection is that
the merger shock wave has passed over an AGN lobe. The shock passing over this
seed population of electrons has led to an increased brightness in the relic
only in the region filled with seed electrons.
