  The unusual morphology of LRG J0239$-$0134 at $z$ =1.062 has been interpreted
as a ring galaxy. Here we propose an alternative idea that the ring-like
morphology is attributed to a pair of superbubbles driven by the intense
starburst in the central region of this galaxy. Supporting evidence for a
superbubble model is; 1) the poststarburst nature in the central body suggests
that a burst of supernova explosions could occur at least $\sim 10^7$ yr ago,
2) the dark lane seen in the central body suggests that we observe this object
from a nearly edge-on view, and, 3) the ring-like morphology is not
inconsistent with an idea that it is a pair of superbubbles. All these pieces
of evidence for the superbubble model seem circumstantial. However, if this is
the case, this galaxy provides an important example of the superwind activity
at high redshift.
