This galaxy presents as an edge-on disk galaxy. There is a prominent central bulge which appears relatively smooth and concentrated. The disk is visible as a faint, extended structure on either side of the bulge, with a noticeable dust lane. There's some indication of potential star formation regions that appear as faint, slightly bluer patches within the disk, most likely due to the dust and gas interaction. The overall morphology suggests a system that is relatively undisturbed, and is relatively dim, indicating a slower star formation rate. Based on the orientation, it is difficult to assess the presence of spiral arms.
