The galaxy presents as a spiral, with a disk-like structure. It is observed at an angle, not quite edge-on, but with a noticeable tilt. The central bulge is prominent, exhibiting a bright, concentrated luminosity, appearing yellowish-white. Spiral arms are evident but somewhat diffuse, winding around the bulge. They appear blueish, suggesting the presence of younger, hotter stars within these arms. Dust lanes are not clearly discernible, though subtle variations in color and luminosity hint at their presence within the spiral arms. The overall appearance indicates a relatively evolved spiral galaxy, possibly of intermediate type.
