The galaxy presents as a spiral, viewed at an oblique angle. There's a noticeable disk component with a central bulge that appears to be moderately prominent. The overall color profile suggests ongoing star formation. Some irregularity can be observed in the disk's structure, suggestive of minor gravitational interactions or internal processes. The morphology is not entirely smooth, indicating either features within the disk, like spiral arms, or some disturbance. The luminosity suggests a massive galaxy. The high star formation rate is notable.
