The galaxy appears as an elliptical morphology, with a smooth, centrally concentrated luminosity profile. It presents with an intermediate ellipticity, neither perfectly spherical nor particularly elongated. There is no apparent spiral arm structure or dust lane features within the visible range. The galaxy's color index suggests a population of older stars, with a reddish hue. The overall structure seems relatively undisturbed, with no immediately obvious signs of a major ongoing merger event, although minor disturbances cannot be ruled out based on visual inspection alone. The diameter of the galaxy indicates that it is a relatively large galaxy. The galaxy exhibits very low rates of star formation.
