The galaxy presents a moderately disturbed morphology. A bright, relatively smooth central bulge is visible, with an apparent tidal tail extending outwards. The color gradient suggests a radial profile with older stellar populations concentrated in the bulge, and hints of bluer, potentially younger stars within the extended tail. The overall color of the galaxy is yellowish, which indicates a population of older stars. The system shows evidence of possible interaction or merger, with the tail potentially formed as a result of tidal forces from a past interaction with another galaxy. There also may be a small, nearby companion galaxy near the bottom left of the image.
