This galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish-orange hue, suggesting an older stellar population. The light becomes more diffuse and redder towards the outer regions. There is no discernible evidence of spiral arms or prominent dust lanes. The overall light profile suggests minimal ongoing star formation, consistent with a passively evolving system. The galaxy appears relatively undisturbed, lacking any obvious signs of recent major mergers or tidal interactions. The shape appears slightly elongated.
