The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated light profile. The light is distributed in a roughly spherical shape, showing a high degree of circularity, without any obvious spiral arm features or a distinct disk component. A faint, diffuse halo extends outward from the central core. There is a smooth color gradient observed, transitioning from a blue-ish center to redder outskirts. The overall appearance suggests a relatively old stellar population, with little ongoing active star formation. There are no obvious signs of tidal disturbances or ongoing mergers.
