The galaxy presents as a centrally concentrated, elliptical-shaped object. The core region exhibits a strong luminosity, with a yellow-white hue. The outer regions show a gradual decrease in brightness, with a subtle transition towards redder tones in the extended halo. There is a high degree of smoothness across the galaxy's light distribution, suggesting a lack of prominent spiral arms or distinct star-forming regions. The overall morphology indicates a galaxy that is likely an early-type system, potentially a massive elliptical with a relatively quiescent star formation rate. Faint disturbances are potentially present, though largely indistinct in the object's morphology.
