This galaxy presents as a relatively smooth, elliptical-like structure. It appears to be dominated by older stellar populations, indicated by the reddish-yellow hue of its central region. The galaxy exhibits a high degree of radial symmetry, with a concentration of light toward the center. There is little evidence of spiral arms or significant dust lanes. The overall morphology suggests a system that has undergone significant dynamical relaxation, possibly the result of past merging events. There may be ongoing or recent minor interactions with smaller nearby systems, as slight distortions in the outer isophotes cannot be fully ruled out. The galaxy appears to have a relatively low star formation rate.
