The galaxy presents as a largely featureless elliptical. The light distribution appears smooth and centrally concentrated, exhibiting a moderate ellipticity. A clear bulge component dominates the morphology. The color gradient suggests an aging stellar population with a relatively low rate of star formation. No distinct spiral arms or significant dust lanes are apparent. There is no evidence of any tidal tails, or ongoing major mergers. The overall appearance indicates a relatively quiescent galaxy which is not currently undergoing significant star formation.
