The galaxy presents as a generally smooth, centrally concentrated object with a spheroidal morphology. A notable feature is its color gradient, transitioning from a more reddish-orange core to a greenish-blue outer halo. The central region exhibits higher surface brightness, suggesting a greater density of stars. The outer regions fade gradually, indicating a decreasing stellar density with increasing radius. There is a very slight hint of disturbed morphology or a minor asymmetry to the light distribution, but the overall structure appears mostly undisturbed. There does not appear to be any significant disk-like structure or spiral arms.
