2 Equulei is a double star system in the constellation of Equuleus.
The primary component of the 2 Equulei pair is an F-type main sequence star. As of 2015, the secondary had an angular separation of along a position angle of 213° from the primary. They form a common proper motion pair, two stars at approximately the same distance and moving in the same direction. Gaia EDR3 gives them parallaxes of and respectively, although they are flagged as potentially unreliable. These parallaxes correspond to a distance of around, in contrast to the Hipparcos distance of for the two stars as a pair.
2 Equulei has been referred to in some sources as λ (Lambda) Equulei, although it was not given that designation by Bayer.