The galaxy presents as a disk galaxy, observed at a moderate inclination. Its morphology is characterized by prominent spiral arms. The disk appears to be the dominant feature of this galaxy. Within the central region is a clear, moderate-sized bulge. The spiral arms appear to be tightly wound. The galaxy is likely a barred spiral, with a prominent bar structure that spans a significant portion of the galactic disk. There is no evidence of any ongoing or recent major merger events. The galaxy shows signs of star formation. 
