This galaxy exhibits a distinct spiral structure. The spiral arms are tightly wound around a bright, moderately sized central bulge. The arms themselves display a blueish hue, suggestive of ongoing star formation activity. The overall morphology is indicative of a galaxy that is not undergoing a major merger, but there is a hint of a slight disturbance in the outer regions of the disk. The galaxy appears to be well-resolved with no noticeable dust lanes. The central bulge displays a less pronounced red color. The morphology seems to be of a late-type spiral galaxy.
