  The Tarleton Observatory's 0.8m telescope and CCD photometer were used to
obtain 1298 observations of the short period eclipsing binary star MW And. The
observations were obtained in Johnson's BVR filters. The light curves show that
MW And is an eclipsing binary star with a period of 0.26376886 days. Further
analysis showed that the period of MW And is changing at the rate of
0.17sec/year. The photometric solutions were obtained using the 2015 version of
the Wilson-Devinney model. The solutions show that MW And is an eclipsing
binary star of W UMa type. Our analysis suggests that the system has a light
curve of W-subtype contact system. Its spectral type of K0/K1, as estimated
from its color, places it in the Zero-Age contact zone of the period-spectral
diagram. Luminosity from the solutions indicate that it is a double-line
spectroscopic system and therefore, spectroscopic observations are recommended
for further detail study.
