The galaxy presents as a fairly smooth, elliptical-like structure. Its overall shape is quite round, exhibiting a high degree of circular symmetry in its light distribution. There's little to no evidence of significant spiral arm structure or prominent disk features.

There is a color gradient visible within the galaxy. The central region appears to be more reddish/yellowish, while the outer regions are subtly bluer in hue. This color difference could indicate a difference in stellar populations, with older, redder stars dominating the core and younger, bluer stars being more prevalent in the outer parts.

There is no obvious visual evidence of ongoing major mergers or tidal disturbances. The light distribution seems relatively undisturbed.
