  We present updated measurements for the position angle and separation of the
double-star WDS 09168-3407 B 1118, incorporating data from our observation,
Gaia Early Data Release 3 mission, and historical records. Our findings
indicate a position angle of 341.4{\deg} and separation of 3.36". Additionally,
we utilized parallax and the ratio of proper motion metric (rPM) values to
evaluate the potential binarity of the system. Our analysis suggests that the
system may be gravitationally bound.
