We present an analysis of multi-epoch low-resolution spectrophotometry , complemented by the light curves provided by massive photometric surveys spanning over 100 years , of the symbiotic binary LMC S63 .
We showed that it is an eclipsing binary with the orbital period of 1050 ^ { d } .
We also found evidence of outbursts in history of the white dwarf .
If it was a Z-And type outburst , as is most likely , it would be a second such outburst recorded in the Magellanic Cloud symbiotic system .
We confirmed that the red giant is enhanced in carbon , and estimated C/O \simeq 1.2 by fitting a model atmosphere to the SALT spectrum .
We also found bi-periodic pulsations of the red giant , and demonstrated that it is similar to other carbon variables with confirmed bi-periodicity .