The galaxy appears as a centrally concentrated object, with a generally smooth, elliptical morphology. The core of the galaxy exhibits a yellowish-white hue, suggesting an older stellar population. The outer regions of the galaxy are fainter and display a slightly bluer tint, potentially indicating the presence of some younger stars, but dominated by an older population. There is no prominent disk structure or spiral arms visible. The overall appearance suggests a relatively undisturbed system, lacking any major signs of ongoing mergers or tidal disruptions.
