The galaxy presents a spiral morphology, exhibiting a well-defined disk structure. Prominent spiral arms emanate from a bright central bulge. The spiral arms display a somewhat flocculent texture with both tightly wound and more open segments. The arms show hints of active star formation, indicated by their bluish hue. The central bulge appears moderately sized, and is elongated. There is evidence of a bar-like structure running through the central region of the galaxy. Overall, the galaxy is relatively undisturbed, though there are slight asymmetries in the outer regions of the disk.
