The observed galaxy appears to be a spiral galaxy, presenting a significant disk component with evidence of spiral arm structure. The arms exhibit a somewhat flocculent morphology. Color gradients within the spiral arms indicate regions of active star formation, with bluer hues. A central bulge is visible, though it does not appear to be the dominant feature of the galaxy. The overall structure seems to show minor disturbances. There is an indication of a bar-like structure spanning the central region, which may be causing some of the disk's disturbances.
