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.
The object is categorized as a proper motion member of the Lower Centaurus–Crux subgroup within the Scorpius–Centaurus OB association; this group is among the nearest clusters of stars that are moving together in space relative to us.