The galaxy appears to be a relatively smooth, lenticular-like object, with a slight elongation. There is a central, bright bulge that exhibits a pinkish hue, indicative of older stellar populations. Extending outwards, there is a fainter disk component that shows a subtle greenish tint. There's no definitive spiral arm structure or dust lanes visible in this image. Overall, the galaxy exhibits a relatively smooth light distribution with a hint of disk morphology. There is a small chance there is a minor disturbance within the disk.
