The galaxy presents as a centrally concentrated spheroid, exhibiting a smooth, featureless morphology. Its overall color appears yellow-orange, suggesting a population of older stars and a relatively low rate of current star formation activity. There is no evidence of spiral arms, bars, or significant dust lanes. The elliptical shape indicates a minimal rotational component and a velocity dispersion dominated system. No tidal tails or distortions are observed, ruling out recent major merger activity, although minor disturbances cannot be discounted.
