The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. Its overall color appears to be yellowish-orange, suggesting a relatively older stellar population and a low rate of on-going star formation. The isophotes show a moderately elongated shape, with a flattening ratio of approximately 0.7. There is a slight apparent warp or twisting of the outer isophotes, hinting at a possible past interaction or merger event, though the overall structure is relatively undisturbed. The galaxy appears to be fairly massive, given its overall size and luminosity. No prominent dust lanes or spiral arm features are discernible in the available imaging.
