The galaxy presents as an elliptical morphology, exhibiting a centrally concentrated bulge that is smooth in appearance. The light profile suggests a well-defined core. The galaxy appears to be relatively isolated, showing no obvious signs of major mergers or tidal disturbances. The color gradient, although subtle, implies a population of older stars concentrated within the central region, with a redder hue toward the core transitioning to slightly bluer colors in the outer halo. The overall structure indicates a galaxy that is evolving passively, potentially with a very low star formation rate. Its size can be described as relatively compact.
