The galaxy presents an elongated, cigar-shaped morphology. It appears relatively smooth in structure, with a central concentration of light that gradually fades towards the edges. Some bluer regions can be seen along the edges and one of the tips, hinting at areas of potentially active star formation. Overall, the galaxy exhibits a reddish-orange hue, suggesting an older stellar population in the central regions. There is a faint, diffuse halo surrounding the main body of the galaxy. No significant signs of a major merger are visible; there may be some minor disturbances in the disk.
