The galaxy exhibits a disturbed morphology, potentially indicative of an ongoing or recent merger event. There is a dominant central bulge with a diffuse, elongated structure extending outward, possibly a tidal tail or distorted disk. The central region presents a strong concentration of light, appearing yellowish in color, suggesting an older stellar population. The outer regions show a bluer hue, hinting at younger, hotter stars, possibly regions of active star formation. The galaxy appears relatively large, exhibiting a measureable diameter. Evidence suggests a significant amount of ongoing star formation, and it's overall mass appears substantial. There's a notable degree of asymmetry and irregularity, supporting the hypothesis of gravitational interaction or merging. The disturbance is significant enough to classify this galaxy as actively merging.
