The observed galaxy presents as a spiral type. High dust content is apparent from the winding and tightly wrapped nature of the spiral arms. A bulge is visible in the center of the galaxy, which appears to be on the smaller side. The arms appear to originate near the central bulge and extend outwards. The spiral arms of the galaxy appear distinct, with a noticeable separation between them. There is also a possible tidal disruption present at the left side of the galaxy.
