The period is uncertain, but it will be a long period variable star. I I-band CCD magnitude observed by the ASAS project. Details are in magnitude data page . The ASAS observations reveal that it is SR-type type with a period of 350 days. John Greaves, UK, identified MisV0823 and ASAS 170101-2249.7.
Details are in magnitude data page .
I-band CCD magnitude observed by the TASS project. The TASS observations for 100 days show it was at maximum. Therefore, it is a long period variable star with a half period of 450 days from maximum to minimum. I-band CCD magnitude observed by the ASAS project. Details are in magnitude data page .