The galaxy presents as a spiral type, observed at a redshift suggesting a relatively distant location. The disk component exhibits well-defined spiral arms. These arms appear to be predominantly tightly wound, with some arms being slightly more medium wound, emanating from a central bulge. The galaxy shows a bar feature that is either weak or absent, with a small-to-moderate central bulge. The disk is oriented at a face-on angle. The morphology of the galaxy suggests that it is not currently undergoing a major merger, but there may be signs of minor disturbance due to past interaction or internal dynamics. The arms display a subtle two-arm structure. The light distribution and color gradients indicate active star formation regions within the spiral arms.
