It is a proper motion member of the Lower Centaurus–Crux sub-group in the Scorpius–Centaurus OB association, the nearest such association of co-moving massive stars to the Sun.
It is a proper motion member of the Lower Centaurus–Crux sub-group in the Scorpius–Centaurus OB association, which is one of the closest groups of co-moving massive stars to our solar system.