The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology is largely elliptical or spheroidal, with minimal apparent disk structure. The color profile suggests an aging stellar population. The core of the galaxy appears yellowish-white, indicating a concentration of older stars. Faint blue hues can be seen further out from the center, possibly indicating some on-going star formation, albeit at a lower rate. The galaxy exhibits no signs of major mergers or significant tidal disturbances, maintaining a regular and largely undisturbed appearance.
