The galaxy presents a distinct spiral morphology with a relatively bright central bulge. Two prominent spiral arms are observed, exhibiting a moderate winding. The arms appear somewhat flocculent, with areas of star formation possibly tracing the spiral structure. The disk is viewed at a slight angle from face-on. The bulge-to-disk ratio suggests a galaxy with a significant disk component. There may be a faint bar structure through the center of the bulge. No significant signs of ongoing major merger events are immediately evident, but there could be minor disturbances. The central region appears bright and likely hosts an active galactic nucleus or a region of intense star formation. Overall, the galaxy appears to be a spiral galaxy with moderate ongoing star formation.
