The galaxy presents as a slightly elongated, disk-like structure. There is a strong central bulge with an intensely bright yellow core, suggesting a high concentration of older stellar populations. The disk appears relatively smooth and displays a gradual decrease in luminosity as it extends outward from the central bulge. Fainter, reddish hues are visible along the outer edges of the disk, indicating the presence of dust lanes and possibly ongoing star formation in these regions. Overall, the galaxy appears to be relatively undisturbed, with no obvious signs of major mergers or tidal interactions.
