The galaxy presents as an elliptical form, exhibiting a smooth, concentrated central bulge that gradually fades into a diffuse halo. The color profile suggests a population of older stars dominating the galaxy's composition, particularly within the central region, as indicated by its reddish-yellow hue. There is no visible evidence of spiral arms or active star formation within the observable portion of the galaxy. The shape is elongated, indicating a departure from a perfectly spherical morphology. The outer regions appear fainter, suggesting a lower stellar density compared to the core.
