This galaxy presents as a spiral type, characterized by prominent, well-defined arms. These arms exhibit a tightly wound morphology, suggesting a relatively old or undisturbed system. The central bulge appears moderately sized, displaying a yellowish hue indicative of an older stellar population. The arms exhibit a bluer color, signifying ongoing star formation. Furthermore, the arms show a structure indicating multiple spiral arms. No signs of a significant bar structure are observed within the galactic disk. Some irregularity in the outer regions suggests a minor interaction or past merger event.
