The observed galaxy presents a morphology consistent with an interacting system. Two primary components are visually discernible. One appears to be a relatively smooth, round component exhibiting a dominant blue hue, possibly indicating ongoing or recent star formation. The second component presents a more orange-red color, and shows signs of disturbance. This could be due to an interaction with the blue component. There is a large overlap of both components, so it can be assumed that they are undergoing a merger. There are no obvious spiral arm structures visible. Overall, the system displays morphological features suggestive of tidal interactions and a late-stage merger event. Further spectroscopic data is needed to confirm. 
