The galaxy presents as an elongated, cigar-shaped structure. The majority of the galactic body exhibits a relatively smooth, diffuse morphology. There is evidence of internal structuring. A color gradient is observed along the major axis. One end of the galaxy shows a reddish-yellow hue which then fades to a bluer coloration towards the opposite end, suggesting variations in stellar populations or dust content. Overall, there is a suggestion of minor gravitational disturbance present.
