The galaxy presents a somewhat irregular morphology, appearing elongated with a distinct, diffuse tidal tail extending outward. The main body exhibits a concentration of light, suggesting a central bulge or core. The color gradient across the galaxy is subtle, with slightly bluer hues in regions coinciding with the tail, which may indicate areas of active star formation. Dust lanes are not distinctly visible, but subtle variations in color suggest their presence. Overall, the galaxy appears to be a disturbed system, possibly resulting from an ongoing or past interaction with another galaxy. The light distribution follows a concentrated profile.
