The galaxy presents as a single, dominant object. It exhibits a smooth, elliptical morphology with a high degree of roundness. There is no visible evidence of spiral arms, bars, or significant disk structures. The galaxy appears to be relatively undisturbed, showing no signs of major mergers or tidal disruptions. The color profile suggests a relatively old stellar population, with a redder hue indicative of less recent star formation. The object is moderately luminous.
