The galaxy appears as a singular, concentrated body of light with a largely smooth morphology. It exhibits a round shape, lacking any distinct features such as spiral arms or a prominent disk structure. The light is fairly uniform across the object, suggesting a relatively homogenous distribution of stellar populations. There is a slight color gradient, shifting from slightly yellower at the core to redder edges, suggesting the presence of older stars. There is no evidence of significant dust lanes or active star formation regions. The galaxy does not appear to be strongly interacting with any other objects in its immediate vicinity, showing no signs of tidal tails or morphological distortions that would indicate an ongoing merger event.
