The galaxy presents a largely face-on spiral morphology. The central bulge appears prominent and has a moderate size relative to the disk. The spiral arms are clearly defined, exhibiting a tightly wound structure. There is evidence of multiple spiral arms extending from the bulge. The galaxy appears relatively undisturbed, showing no significant signs of a major merger event. A weak bar structure may be present across the bulge. Overall, the color profile indicates ongoing star formation within the spiral arms, exhibiting bluer hues, while the central bulge appears more yellow/red, indicative of an older stellar population.
