The galaxy appears as a centrally concentrated, smooth object. Its color is predominantly yellow-white in the central region, suggesting an older stellar population. The morphology suggests an elliptical or lenticular galaxy type, with little evidence of spiral arms or significant dust lanes. The galaxy exhibits a slight elongation, deviating marginally from perfect circularity, though it is mostly round. There is a subtle fading of the luminosity from the core outwards, with no obvious signs of recent major merger events or tidal disturbances. The absence of distinct blue regions indicates a low ongoing star formation rate.
