The galaxy presents as a smooth, centrally concentrated object. There is an absence of spiral arms or a well-defined disk. The light distribution appears relatively uniform, with a gradual decrease in intensity from the core outwards. It possesses a round morphology with an apparent overall yellowish hue. The galaxy shows no signs of major disturbances or ongoing merger activity in this image, but a minor disturbance cannot be ruled out. Based on the observed color and morphology, this is likely a galaxy that has largely ceased significant star formation activity.
