The galaxy presents as a cigar-shaped, elongated structure. It appears to be relatively smooth, but there is a slight hint of a disk or some type of visible feature. No significant merging or disturbances are apparent, though a minor disturbance cannot be ruled out. The color distribution suggests a possible redder core region transitioning to slightly bluer outer regions. While the galaxy appears largely uniform, closer inspection reveals some subtle color variations indicative of differing stellar populations or dust content across the structure.
