The galaxy presents an overall irregular morphology. A diffuse, elliptical halo surrounds a brighter, more concentrated central region. The core exhibits a bluer color, suggestive of recent star formation or an active galactic nucleus. Fainter, extended structures are visible, potentially tidal tails or remnants of a past interaction or merger event. The color distribution across the galaxy is not uniform, with subtle variations hinting at differing stellar populations or dust content. A slight distortion in the outer regions indicates the possibility of gravitational interaction or internal dynamic processes. Overall, this galaxy appears to be either in a state of disturbance or is composed of a smooth profile galaxy and nearby light sources that are creating a false image. 
