 YZ CMi is a potential member of the Beta Pictoris moving group.This is a red dwarf star, or M-type main-sequence star, with a stellar classification of M5 V. It is a flare star, so called due to its solar flares being more powerful than those of Earth's star, and is roughly three times the size of Jupiter.The radio emission from the star is in a 50 mHz bandwidth and is centered on 1464.9 mHz.