This galaxy exhibits a smooth, elliptical morphology. The central bulge is prominent, displaying a yellowish hue, which may indicate an older stellar population. There is a gradual decrease in luminosity from the core outwards, suggesting a diffuse halo. The overall shape of the galaxy appears elongated, rather than perfectly spherical. No distinct spiral arms or significant dust lanes are visible. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. A slight blue tinge is visible on the outer edges of the disk, potentially suggesting areas of relatively higher star formation.
