The galaxy presents a disturbed morphology, suggesting an ongoing or recent interaction with another galaxy. The primary body of the galaxy exhibits a diffuse, irregular shape with no clearly defined spiral arms or elliptical structure. There appears to be a tidal tail or stream extending from the main body, indicating gravitational disruption. Color variations within the galaxy suggest a mix of stellar populations. A blue hue is visible in parts of the galaxy, possibly indicating regions of active star formation. Overall, this galaxy appears to be undergoing a merging event or experiencing significant gravitational disturbance.
