The galaxy exhibits a disk-like morphology, displaying spiral arm structure. A central bulge is observed, and it appears moderate in size. The presence of a bar feature is evident within the central region of the galaxy, showing a structure that spans a significant portion of the bulge. The spiral arms appear somewhat flocculent, extending from the bar, and exhibit varying degrees of tightness. There are no obvious signs of major mergers, interactions, or significant disturbances in the overall structure of the galaxy. The disk appears to be at a moderate inclination with respect to our line of sight. The color distribution suggests ongoing star formation.
