Background originating from events outside of the interaction point is going to play a major role in the upcoming Belle II experiment. In order to reduce this background a track trigger based on the reconstruction of an event's z position is employed on FPGAs. This paper presents the architecture and implementation of neural networks and supporting preprocessing that is going to be used at the upcoming cosmic ray test of Belle II. By using hit information from simulations, figures of merit like latency and resource demand are presented.