The galaxy presents a primarily smooth morphology, appearing as an elongated, cigar-shaped structure. A subtle color gradient is observed, shifting from blue at one end of the galaxy to a redder hue at the opposite end. The overall shape suggests that the galaxy is either a highly elongated elliptical galaxy or a disk galaxy observed edge-on. No distinct spiral arms are apparent, supporting the notion of a smooth profile. There are no clear signs of a major ongoing merger, although there are faint hints of minor disturbances in the shape. The galaxy exhibits a faint blue glow, indicating potential on-going star formation.
