The galaxy presents as an edge-on spiral, with a prominent and concentrated central bulge. A thin disk extends outwards from the bulge. The bulge exhibits a somewhat rounded morphology. There are signs of some disturbance or asymmetry within the galaxy. The disk has a redder hue closest to the bulge and is somewhat bluer towards the outskirts, consistent with ongoing star formation within the disk. The galaxy is of significant mass, with a moderate star formation rate.
