The galaxy presents as a somewhat smooth, centrally concentrated object, possibly an elliptical or S0 type. There is some evidence of subtle features, though the overall morphology appears relatively undisturbed. The isophotes are roughly elliptical, with a slight elongation. The galaxy exhibits a color gradient, appearing redder toward the center and bluer in the outer regions, suggesting a decreasing age of stellar populations with increasing distance from the core. There is no apparent spiral arm structure or a prominent disk. There is some evidence of minor disturbance.
