The galaxy presents as a central, somewhat smooth and amorphous structure with a slight elongation. A faint tidal tail appears to extend from the main body, suggesting a possible past interaction or ongoing gravitational disturbance. The color profile shows a mix of older stellar populations as well as some ongoing star formation, particularly concentrated in the central region and possibly within the tidal tail itself. Overall, the morphology suggests a galaxy that has experienced some form of disruption, but is not undergoing a major merger. It is neither a pure elliptical nor a well-defined spiral.
