The galaxy presents as a centrally concentrated, elliptical system. Its morphology appears largely smooth with no apparent spiral arm structure or prominent dust lanes. Color gradients suggest a redder core transitioning to slightly bluer outer regions. There is no obvious tidal debris or interaction with other galaxies, indicating it is currently undisturbed, perhaps having undergone a merger a long time ago and relaxed since. Its overall round shape and high level of smoothness suggest a significant population of older stars relative to younger blue ones. The yellow/red-shift color implies considerable distance. Given the limited resolution, finer details are difficult to ascertain.
