The galaxy presents a smooth, elliptical morphology. A concentrated central bulge exhibits a yellow-orange hue, suggestive of an older stellar population. Moving outward from the core, the color transitions to a faint greenish-blue tint, indicating the possibility of some ongoing, albeit subdued, star formation in the outer regions. The overall shape is neither perfectly spherical nor highly elongated, appearing somewhere in between. There are no obvious signs of major mergers or significant tidal disturbances. The galaxy appears relatively isolated and relaxed in its structure.
