The galaxy presents a morphology indicative of a system undergoing a merger event. The central region exhibits a concentrated, bright, and somewhat diffuse profile. The overall light distribution is not entirely smooth, displaying some irregularity. There is an asymmetrical elongation or tidal feature extending from the main body, suggesting gravitational interaction with another system or internal disruption. The colour gradients show a general trend of a redder center, and slightly bluer outer regions. This could imply different stellar populations are present. 
