The galaxy presents as a centrally concentrated elliptical with a smooth morphology. It exhibits a high degree of radial symmetry, appearing nearly round. The galaxy's light is dominated by a prominent bulge, which fades gradually into a diffuse halo. There is no visible dust lane or spiral structure. Color gradients suggest a redder core transitioning to slightly bluer hues in the outer regions. No prominent tidal features or signs of recent major mergers are apparent, although some minor disturbance cannot be ruled out given the slight asymmetry in the outer halo. Overall, the galaxy appears to be a relatively evolved system.