The galaxy presents as a disk-shaped system, appearing elongated with a high aspect ratio. The central bulge exhibits a strong yellow hue, suggesting a population of older stars. The disk component surrounding the bulge shows hints of bluer regions, especially at the edges, indicative of some ongoing star formation. The galaxy appears relatively smooth, with no obvious spiral arm structure visible in this image, although the color variations suggest some internal structure within the disk. There is no evidence of a major ongoing merger or significant tidal disruption.
