The galaxy presents as a generally elliptical object with a somewhat smooth appearance. The light distribution appears relatively uniform. The central region presents as slightly more concentrated than the edges of the observed shape.

The object displays a subtle color gradient, shifting from a slightly bluer hue at the center, trending toward more red or orange at the periphery. This might indicate younger stellar populations are concentrated towards the center of the galaxy.

There are some indications of irregularities or small disturbances, such as minor variations in color or light distribution, but these are not indicative of major mergers or strong tidal interactions. The primary structure of the galaxy seems to be largely undisturbed.
