The galaxy presents a distinct spiral structure, exhibiting prominent, well-defined arms. These arms are traced by regions of active star formation, indicated by their bluer color. The winding of the spiral arms appears to be of medium tightness. The galaxy appears to be disk-dominated and not particularly bulge-dominated. There may be a central bar structure. Overall, it's a prominent disk galaxy undergoing star formation, with no apparent major merger events or significant tidal distortions. The luminosity of the disk is significant. The morphology is fairly regular.
