I think the answer is yes. There is a mira variable called V1951 Sgr that is very close to the area you ar looking at. It is a bit blurry to be certain and it is a very busy field. Your image is oriented west up and south to the right.
The mira ranges from about mag 8 to 15 over a 510 day cycle.
Curiously it is not exactly where it is catalogued. I have looked in the catalogues an dcompared them to the DSS filed and one of my images. The star you have seen is on the DSS images and on my image (marked) but the catalogued position is not on the DSS image or my image. I assume it is either an error or the star has a high propper motion.
I have rotated my image to match your one.
The DSS image with the variable marked is
here.