Magakian et al. (2019) called attention to the current bright state of LkHa 225 South, which over past two decades has changed from $>20^m$ $<13^m$. We present recent optical photometric monitoring that shows colorless, non-sinusoidal, periodic brightness variations. The oscillations occur every 43 days, and have amplitude $\sim$0.7 mag with some variation among cycles. also new flux-calibrated...