The galaxy presents a relatively smooth, elliptical morphology. The core exhibits a concentrated, bright yellowish-white light, indicative of an older stellar population. The galaxy's shape is generally round, with slight elongation. There are no obvious spiral arms or prominent dust lanes. No apparent signs of major mergers or tidal disturbances are observed. The faint blue fringe surrounding the central region could indicate pockets of younger stars or residual star formation. The galaxy exhibits a relatively smooth light profile overall.