The galaxy presents as a relatively smooth, elliptical-like structure. There is a slight elongation, but it largely appears spheroidal. The color gradient appears to be somewhat uniform across the galaxy, with a subtle shift towards redder hues in the central regions and slightly bluer in the outskirts, suggesting older stellar populations are centrally concentrated and younger stars are more distributed in its halo. The galaxy appears mostly undisturbed, with no obvious tidal features or signs of a recent major merger. There may be subtle asymmetry.
