The galaxy exhibits an irregular morphology, suggesting an ongoing or recent interaction or merger event. The primary body of the galaxy appears relatively smooth, with a somewhat rounded shape, although some asymmetry is present. There is evidence of tidal features or minor disturbances in the form of faint extensions, indicating potential gravitational interactions with another galaxy. The color distribution shows a mixture of stellar populations. The central regions display a yellowish-orange hue, suggesting older, cooler stars and/or significant dust content. The outer regions exhibit bluer colors, which could indicate regions of more recent star formation containing younger, hotter stars. Overall, the galaxy's morphology and color distribution suggest a dynamic system undergoing significant evolutionary processes.
