The galaxy appears to be a spiral galaxy viewed at an oblique angle. It exhibits a prominent, tightly wound spiral arm structure. The arms display a mottled texture, suggesting areas of active star formation. A central bulge is visible, appearing relatively small compared to the disk. The galaxy shows evidence of a bar structure running through the central region. The dust lanes are not very prominent in the image. The galaxy appears to have a moderate inclination. Overall, the galaxy exhibits a blueish hue suggesting ongoing star formation activity.
