The galaxy appears to be a spiral galaxy undergoing a significant interaction or merger. The central bulge is moderately bright and somewhat diffuse, with a slight elongation suggesting a disk component viewed at a moderate inclination. Faint spiral arms are hinted at, exhibiting a patchy structure, possibly due to ongoing star formation. There are indications of tidal features or distortions, seen as faint extensions or irregular shapes surrounding the main body of the galaxy, with a disrupted morphology, indicative of a past or ongoing merger event. Overall, this galaxy presents a dynamic, possibly transitional state, suggesting ongoing evolution driven by external interactions. The color suggests a bluer hue with some active star formation.
