The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology appears largely elliptical, with a high degree of roundness. There may be a very slight indication of a disk structure, but this is difficult to ascertain from the image. The galaxy exhibits a color gradient, with a bluer core region transitioning to redder hues in the outer regions. There are some indications of minor disturbances in its morphology. The galaxy is not completely uniform and may be interacting with another galaxy, but this disturbance may also be due to internal processes.
