The galaxy exhibits a generally elliptical morphology, although irregularities are present in its overall shape. A bright, concentrated central region, likely the galactic nucleus, is observed. The galaxy appears to be composed of a diffuse distribution of stellar populations. The central core is blueish. Some color gradients are observed, with bluer hues towards the center and slightly redder hues in the surrounding regions. Overall, the galaxy appears relatively smooth, but there is a hint of a disk-like component. There are signs of minor disturbances and some evidence that a merger event took place. The galaxy also appears to be surrounded by a faint halo.
