The galaxy presents a distinctly elongated, cigar-shaped morphology. It appears to be a disk galaxy viewed at a high inclination, close to edge-on. A central bulge, exhibiting a yellowish hue, is visible. The disk component appears bluish, suggesting the presence of relatively younger stellar populations and ongoing star formation. The galaxy lacks any obvious spiral arm structure or bar. No signs of recent major merger activity is visible. The galaxy shows some minor disturbance. There is some asymmetry in the disk's overall shape, perhaps caused by tidal interactions with another galaxy.
