The galaxy presents a largely smooth and rounded morphology. It appears as a concentrated, centrally bright object, with a gradual falloff in luminosity towards its outer regions. There is a slight elongation away from the central regions, but this is very minor. The color gradient suggests a composition of older stellar populations, with a dominance of redder hues. Faint blue hints in the outer regions possibly indicate some ongoing, albeit subdued, star formation. No distinct spiral arm structure or prominent dust lanes are visible. The galaxy does not show any strong evidence of tidal disturbances or interactions with other galaxies.
