The galaxy appears to be a relatively smooth, disk-like structure, viewed at an oblique angle. The central region exhibits a high degree of concentration, suggesting a prominent bulge component. The color of the central bulge appears more yellowish-red than the outer disk. The outer regions display a bluer hue, possibly indicating the presence of younger stellar populations and ongoing star formation within the disk. The galaxy does not exhibit any obvious spiral arm structure or bar. There is no indication of major disturbances or merging activity in this image, although the overall shape is elongated. There is a hint of some patchiness within the outer regions of the disk, which may indicate areas of higher star formation or dust concentration.
