The galaxy presents as a spiral type, observed at an oblique angle relative to its galactic plane. A prominent central bulge dominates the core region, appearing yellowish-orange. The spiral arms exhibit a moderately wound structure, with at least two clearly discernible arms emanating from the central bulge. The arms themselves demonstrate a mottled appearance, suggesting regions of active star formation and dust lanes. There is some evidence of minor disturbances in the morphology, possibly indicating an ongoing interaction or a recent merger event. The galaxy exhibits a relatively high disk to bulge ratio, indicative of it being a relatively active spiral galaxy.
