The galaxy presents as a centrally concentrated object with a roughly elliptical morphology. The core region exhibits a pronounced yellowish-orange hue, suggesting an older stellar population and possibly a higher concentration of dust. The outer regions appear somewhat fainter and more diffuse, with a subtle gradient in color transitioning toward redder tones. There is little evidence of distinct spiral arm structures or significant star formation regions within the observable extent of the galaxy, implying it's a relatively passive galaxy. The overall smoothness of the light distribution supports the interpretation of it being an elliptical galaxy that appears undisturbed.
