WX LMi is a very low accretion Polar - possibly a pre-Polar (detached system) with accretion from the wind rather than mass transfer from secondary.  The high state level is unknown, and is the primary reason for monitoring.

 

CCD observations obtained with the Bradford Robotic Telescope, and V-band observations obtained with the Sonoita Research Observatory 35cm and 50cm telescopes (through the AAVSO).