The galaxy presents as a spiral galaxy with a notable central bulge. Spiral arms are visible, extending from the central region, though the resolution limits precise characterization of their structure. The orientation suggests the galaxy is viewed at an angle, but not edge-on. There is a possible presence of a bar feature within the central region of the galaxy. The disk component appears complex with a lumpy nature, possibly indicative of ongoing star formation regions, which could be signs of merging activity. There is also a disturbance within the galaxy's structure, and the presence of tidal features cannot be ruled out.
