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 0.17 sec / 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 type diagram .
Luminosity from the solutions indicates that it is a double-line spectroscopic system and therefore , spectroscopic observations are recommended for further detail study .