The galaxy presents as an elliptical morphology, appearing largely smooth and featureless. Its shape is somewhere between round and elongated. The color profile is predominantly yellowish-orange toward the center, suggesting an older stellar population. A slight gradient toward greenish-blue hues can be observed at the outer edges, possibly indicating the presence of younger stars or ongoing, albeit limited, star formation in the outer regions. There's no obvious evidence of a strong, actively star-forming disk, or any major ongoing merger activity. The galaxy appears to be a relatively isolated system based on the lack of visible tidal distortions or close companions.
