The galaxy presents a largely smooth and elliptical morphology. Its light is concentrated towards the center, which exhibits a bright, nearly circular core. The core's light appears to gradually fade as it extends into the galaxy's outer regions. There are some very faint hints of bluer light suggesting a small degree of star formation. Overall, the galaxy appears well-formed and relatively undisturbed, without any obvious signs of ongoing or recent major mergers. The galaxy shows a high degree of central light concentration, suggesting a significant bulge component.
