The galaxy appears as a single, concentrated object. It presents a generally smooth morphology, indicative of an elliptical galaxy or a spiral galaxy viewed face-on at a considerable distance. There is little discernible spiral arm structure or irregular features. The galaxy displays a distinct blue hue in the center, which suggests the presence of younger, hotter stars and potentially ongoing star formation within this region. The galaxy exhibits a fairly uniform color profile, transitioning to slightly redder tones towards its outer edges. It shows a high degree of circularity. There's no obvious evidence of major tidal disturbances or merging activity. The object presents as a singular, relatively undisturbed galactic structure.
