The galaxy appears as a centrally concentrated, relatively smooth object. It exhibits a predominantly elliptical morphology, with a high degree of radial symmetry. There is a slight deviation from perfect circularity, leaning towards an intermediate shape. No prominent spiral arm structures are discernible. There is a hint of minor disturbances in the galaxy's structure, although a major merger is not indicated. The light profile suggests an older stellar population, which is consistent with the lack of blue light. The overall color is slightly redder, indicating that recent star formation activity is low. The overall impression is that of a well-formed, evolved galaxy, possibly nearing the quiescent stage of its evolution.
