The galaxy appears as a centrally concentrated, elliptical-like object. It exhibits a smooth, featureless morphology, lacking any discernible spiral arms or bar structures. The color profile indicates a dominant yellow hue in the central region, possibly indicating an older stellar population, with a gradual transition to a redder shade at its outer edges. The light distribution suggests high degree of rotational symmetry, with no prominent asymmetries or tidal features, with only very slight disturbances. The galaxy is well-defined with no signs of a merging event, despite its considerable size and mass. The overall impression is that of a well-evolved, early-type galaxy exhibiting a quiescent star formation rate.
