The galaxy presents a largely elliptical morphology, appearing relatively smooth and concentrated. There's a high degree of rotational symmetry, showing minimal deviation from a circular shape. I find no obvious signs of spiral arms, a bar structure, or any significant disk-like features. Nor does the object appear to be undergoing any active merging events or displaying tidal tails, plumes, or other substantial distortions. The galaxy exhibits a color gradient, transitioning from a brighter, more yellow/orange central core to a dimmer, slightly redder halo. This suggests a possible aging stellar population and low levels of star formation. The overall light profile is consistent with that of a massive galaxy.
