The galaxy presents a well-defined spiral structure with multiple arms emanating from a central bulge. The spiral arms are tightly wound, exhibiting a somewhat flocculent morphology with regions of enhanced star formation evidenced by a bluer hue in those regions. The central bulge appears relatively small and is a bright source of light. There is some evidence of a weak bar structure present within the central region of the galaxy. The overall color suggests an actively star-forming disk, though no significant signs of a major merger event are visible in this image; some minor disturbances may be present. The disk is viewed nearly face-on.
