The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, with no discernible spiral arm structure or bar. The central region is brighter and appears yellowish, suggesting a population of older stars. The outer regions fade gradually, with a slightly bluer tint compared to the core. This subtle color difference could indicate a small amount of ongoing star formation, though the overall appearance suggests it's a relatively quiescent system. There is no evidence of major mergers or tidal disturbances in the image.
