This galaxy appears to be a spiral type, exhibiting a prominent disk structure. Spiral arms are visible, although not sharply defined, showing a somewhat flocculent pattern. The arms display a bluish tint, suggesting ongoing star formation. The central bulge is not overly pronounced and presents a yellowish-orange hue, potentially indicating an older stellar population. There's a hint of dust lanes within the disk, though not particularly prominent. The galaxy is not perfectly face-on, offering a slightly oblique view of its features. Overall, it appears to be a typical spiral galaxy with moderate star formation activity and a relatively normal bulge-to-disk ratio.
