An eclipsing variable star similar to Algol has a period of 2.32 days and its brightness ranges from 4.92 to 5.9 magnitude. The entire cycle of brightness changes can be observed with the naked eye. The change from maximum to minimum occurs in about 6 hours, which can be noticed in a single spring night. Among the main minima, there is one insignificant secondary minimum, which only reaches a tenth of the stellar magnitude, making it difficult to perceive. The system is located nearly 300 light-years away from Earth.