The galaxy presents as a structure with features suggesting an ongoing or recent merger event. There are at least two distinct light concentrations, indicating possible galactic nuclei. The primary concentration appears more diffuse with a yellowish hue, possibly indicating an older stellar population and lower levels of star formation. The secondary concentration exhibits a more compact structure with a slightly redder hue, potentially suggesting ongoing star formation or dust obscuration. There is a faint tidal tail or bridge of material extending between the two concentrations, which could also be due to the interactions between the two merging galaxies. The overall morphology is irregular, consistent with a system undergoing gravitational disturbance. Based on the colours in the image, the stellar population is likely a mix of older and intermediate-aged stars, with pockets of younger stars.
