The galaxy presents a spiral morphology, with a relatively bright central bulge exhibiting a yellowish hue. The spiral arms are well-defined, displaying a tightly wound structure that suggests a relatively evolved system. Dust lanes appear to be present within the arms, contributing to the observed patchy texture and obscuring some of the light from the underlying stellar populations. The arms exhibit a bluish tint, indicative of recent star formation activity, with the inner arms showing somewhat less of this bluish hue than the outermost regions of the galaxy. The galaxy shows signs of interactions or mergers in its morphology as there are significant distortions apparent.
