The galaxy presents a largely smooth, elliptical morphology. It exhibits a bright, concentrated central bulge that appears yellowish in color, suggesting an older stellar population. Extending outward from the bulge is a fainter, more diffuse halo that displays a bluish tint. This might indicate the presence of some younger, hotter stars, but overall the halo seems dominated by older stars as well. No distinct spiral arm structures or significant dust lanes are visible. The galaxy appears relatively undisturbed, with no obvious signs of ongoing major merger activity or tidal distortions.
