The galaxy appears as a centrally concentrated, luminous spheroid. It exhibits a smooth, elliptical morphology with no discernible spiral arm structure or distinct features. The color gradient transitions from a bright, yellowish core to a more subdued, reddish outer halo. The galaxy's overall shape is moderately elongated, deviating slightly from a perfectly circular form. There is no evidence of ongoing mergers or major disturbances, although a minor irregularity in the outer regions may suggest past gravitational interactions. Based on its smooth morphology, it can likely be classified as an elliptical galaxy with moderate mass and a low specific star formation rate.
