The galaxy presents a generally smooth, elliptical morphology. Its color profile suggests an older stellar population, with a dominant yellowish-orange hue concentrated towards the central region. A subtle greenish tinge is observed at the periphery, potentially indicative of some ongoing, albeit limited, star formation activity. The overall shape is somewhat elongated, with the galaxy appearing more cigar-shaped than perfectly spherical. There is no evidence of major mergers or significant tidal disturbances in its immediate structure, although a minor asymmetry cannot be ruled out.
