This galaxy exhibits a flattened, elongated morphology. There's a concentration of light in the center, appearing somewhat yellowish-white. The outer regions display a more diffuse, bluish hue, suggesting the presence of younger stellar populations and ongoing star formation. The overall structure appears relatively smooth, with some hint of possible disturbances or faint features in the disk, although no clear spiral arm structure is visible. The elongation suggests it could be classified as a cigar-shaped or lenticular galaxy. There's a slight asymmetry in the light distribution of the outer regions, which could indicate possible past or ongoing interactions.
