The galaxy presents as a centrally concentrated object with an elliptical morphology. The light distribution appears smooth, lacking any prominent spiral arm structures or distinct features. There is a gradual decrease in luminosity from the core outwards, indicating a centrally dominant bulge. The ellipticity of the galaxy is moderate, appearing somewhere between round and elongated. No signs of tidal disturbances, major mergers, or significant star formation regions are apparent in the image. The color gradient suggests an older stellar population, with a yellowish hue dominating the galaxy's overall color.
