The galaxy presents a largely smooth, elliptical morphology. There is a centrally concentrated bulge that gradually diffuses outward into a fainter halo. The galaxy exhibits a color gradient, shifting from a slightly redder core to a bluer periphery. There is no apparent spiral arm structure or distinct dust lanes. The overall appearance suggests a relatively evolved system, with evidence of minimal ongoing merging activity. It shows limited evidence of major disturbances. The isophotes are generally regular, displaying a deviation from a perfectly circular shape, indicating an intermediate elliptical form.
