This galaxy exhibits a flattened, elliptical morphology, appearing as a disk-like structure viewed at an oblique angle. The central bulge is prominent and exhibits a smooth, concentrated light profile, suggesting an older stellar population. The outer regions of the galaxy display a fainter, less structured distribution of light. There's an apparent minor asymmetry and irregularity in the disk suggesting possible gravitational interaction or internal dynamics influencing its shape. Faint, diffuse spiral arm structures may be present, although resolution limitations hinder definitive classification. Color gradients suggest variation in stellar populations across the galaxy, with the bulge appearing redder and the disk exhibiting bluer hues.
