The galaxy presents a complex morphology, appearing to be in a state of interaction or merger with another galactic object. A larger, diffuse component displays a yellowish hue, suggesting an older stellar population and a relatively low rate of current star formation. The shape of this component is somewhat elongated. A smaller, more compact component is noticeable, exhibiting a bluer color, indicative of younger, hotter stars and active star formation. There seems to be some morphological disturbance present within the system. Given the appearance, a potential scenario includes a relatively large galaxy undergoing interaction, possibly a merger, with a smaller, gas-rich companion. 
