The galaxy presents a morphology suggesting an ongoing or recent merger event. Two distinct, luminous cores are visible, indicative of the nuclei of the merging galaxies. The overall shape appears elongated, with an elliptical-like profile, but distorted due to the interaction. Faint tidal features or extended arms are not clearly discernible from the image, likely indicating these features are beyond the detection capabilities. The colour profile suggests a mixture of stellar populations with younger, bluer stars present alongside older, redder stars, but these colour differences are not strong. The galaxy is moderately luminous, suggesting a significant stellar mass. Given the merging state, any ongoing star formation is likely suppressed. 