The galaxy appears to be relatively smooth and elliptical in shape, with a centrally concentrated bright core. A disk structure can be inferred, but is faint. There is a noticeable color gradient, shifting from bluer hues in the central regions to redder tones in the outer halo. No strong spiral arm structures or significant dust lanes are visible. The overall impression is of an evolved system, with a possible inclination with respect to our line of sight. There appear to be some minor disturbances and there are features possibly indicating a merger.