This galaxy exhibits a disturbed morphology, appearing to be in a late-stage merger with a smaller companion galaxy. A dominant, somewhat centrally condensed component displays a yellowish hue, suggesting an older stellar population and reduced ongoing star formation. This main component shows some evidence of tidal features or distortions. The smaller companion has a bluer color, indicative of more active star formation. The overall shape of the system is irregular, lacking a well-defined disk or spiral structure. There is a hint of faint, extended tidal tails or debris surrounding the system, indicative of gravitational interaction between the galaxies.
