The galaxy presents a distinctly elongated, cigar-shaped morphology. The light distribution appears relatively smooth. The central region exhibits a yellowish hue, possibly indicating an older stellar population. Extending outwards from the central bulge, the color shifts to a bluer tone, which may be indicative of ongoing star formation within the galactic disk. No prominent spiral arm structures or significant dust lanes are discernible in the image. The overall structure suggests a disk galaxy viewed at a high inclination, nearly edge-on. There is no evidence of any major ongoing mergers. There may be some minor disturbance in the disc.
