The galaxy appears to be undergoing a major merger, exhibiting significant morphological disturbance. There are two distinct light concentrations that are likely the cores of the merging galaxies. The northern core exhibits a yellowish hue, suggesting a population of older stars and/or significant dust obscuration. The southern core presents a bluer color, potentially indicating ongoing or recent star formation activity. The overall shape is highly irregular, deviating significantly from an elliptical or spiral morphology. A faint tidal tail or bridge appears to be present, extending outward from the system, further supporting the ongoing merger scenario. Based on the observed color distribution and disturbed morphology, this galaxy merger is actively influencing the star formation rate within the system.
