The galaxy presents a distinct spiral morphology. The arms appear relatively loosely wound and extend outwards from the central region. A small bulge is suspected, but it is difficult to distinguish it from the disc of the galaxy. There appears to be no strong bar feature. Some signs of minor disturbances can be observed in the galaxy shape, likely caused by an ongoing or recent merger event. The galaxy exhibits colour variations, with bluer hues observed in the spiral arms indicative of ongoing star formation. Overall, the galaxy is a spiral galaxy undergoing active star formation, with potential disturbances from a minor merger.
