The galaxy presents as a single, centrally concentrated luminous object. Its morphology appears largely smooth and elliptical, with a high degree of circularity. The galaxy exhibits a dominant bulge component, characterized by a smooth radial light profile that decreases in intensity from the center outwards. The color is generally yellow, suggesting a population of older stars. There is no apparent spiral arm structure, bar, or distinct dust lanes visible in the image. There is no evidence of tidal features, major disturbances, or ongoing merger activity.
