The galaxy presents a flattened, elliptical morphology, suggesting a disk-like structure viewed at an oblique angle. A central bulge is apparent, exhibiting a higher concentration of light and a yellowish hue. Moving outward from the core, the disk component displays a more diffuse light distribution with some evidence of bluer components. There appears to be minimal indication of defined spiral arms or significant irregular features within the galaxy. The overall color profile indicates a higher concentration of older stellar populations residing within the central region of the galaxy.
