The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core is bright and exhibits a yellowish-orange hue, suggesting an older stellar population. Surrounding the core is a fainter, bluer halo or disk-like structure, indicating the presence of some younger stars and potentially ongoing, albeit subdued, star formation. The overall structure is regular, with no obvious signs of major mergers or significant tidal disturbances. There is a very slight hint of a possible spiral structure, but it is not well-defined. The galaxy appears relatively isolated, with no immediately interacting neighbors in the immediate vicinity.
