The galaxy presents an overall elliptical morphology, appearing relatively smooth and concentrated towards its center. The light distribution suggests a dominant spheroidal component, with little to no discernible spiral structure. There is a slight elongation, though it appears mostly round. The core region exhibits a pronounced, bright concentration indicating a possible active galactic nucleus (AGN) or a dense stellar population. A subtle color gradient is visible, with the central region exhibiting warmer tones in the yellow-orange spectrum, which could indicate an older stellar population or the presence of dust. Fainter blue tinges are noticeable in the outer regions, potentially indicating the presence of younger, hotter stars albeit at a lower rate. The absence of prominent tidal features or nearby companions suggests that it has experienced no recent major merger events. The galaxy appears relatively undisturbed and evolved.
