The galaxy appears to be a ring galaxy. The central region exhibits a yellowish hue, suggesting an older stellar population, possibly a significant bulge component despite appearing relatively small. A distinct, well-defined ring of bluish light surrounds the core, indicating active star formation. The ring structure shows some clumpy formations, potentially denoting regions of increased star formation. The overall structure seems complex, potentially influenced by gravitational interactions or a past merger event. Faint, tightly wound spiral arms or disrupted disk features may be present within the ring, though obscured by the brightness of the surrounding ring. There is no apparent bar structure.
