Based upon the position and movement of this star through space, it is a likely member of the Gould Belt. In particular, it belongs to the Lower Centaurus–Crux (LCC) group of the Scorpius–Centaurus association, which is the nearest OB association to the Sun.
Based on the star's position and movement in space, it is probable that it belongs to the Gould Belt. Specifically, it is part of the Lower Centaurus–Crux (LCC) subgroup within the Scorpius–Centaurus cluster, which is the closest OB group to the Sun.