We present the first analysis of photometric observations of NSVS2607629.
New light elements was obtained and found that the system is located near the short-period limit.
We present method of getting crucial information about spot parameters.
Secondary minima did not occur at phase 0.5P like the systems V407 Peg, LU Vir and HH Boo.
The geometrical and physical parameters of the system were derived.