The galaxy exhibits a complex morphology with a possible ongoing merger event. The central region displays a somewhat smooth appearance, however, this is disturbed by noticeable features. There is a distinct elongation with diffuse and irregular structures extending from the main body. These extensions may be tidal tails and indicate gravitational interaction with another galaxy or a recent merger. Color variations suggest differing stellar populations or dust obscuration within the galaxy. The blue hue in some regions could signify active star formation. There is a noticeable area to the top right of the core that appears to be a significant disturbance, perhaps even a smaller, merging galaxy. While the overall structure is ambiguous, the evidence suggests a disturbed system undergoing interaction.
