The galaxy presents an irregular morphology, possibly indicative of an ongoing or recent merger event. It appears to be a system with multiple components. There is a central, somewhat diffuse region that seems relatively smooth. Extending from this is a more elongated feature, possibly a tidal tail or distorted spiral arm. The color gradients suggest differing stellar populations within the galaxy. Some regions display bluer hues, which could be indicative of younger, hotter stars and active star formation. Other regions have a redder color, potentially indicating older stellar populations or dust obscuration. The overall system appears moderately luminous, suggesting it is a fairly massive galaxy. The degree of disturbance in its structure suggests significant interactions affecting its morphology and likely influencing its star formation rate.
