The galaxy appears to be a relatively smooth, elliptical-like structure. It has a concentrated central bulge with a yellow-orange hue, suggesting an older stellar population likely dominated by evolved stars. Surrounding the bulge is a fainter, diffuse halo that fades into the background. The halo exhibits a subtle blue-green tinge, possibly indicating the presence of some younger stars or ongoing, albeit subdued, star formation within its outer regions. There is a slight asymmetry to the galaxy’s overall shape, with a possible minor disturbance or faint tidal feature extending from one side. While no prominent spiral arms or distinct disk features are visible, the overall morphology indicates a mature galaxy that may have undergone some past interaction or minor merger. The central region appears dense and well-defined, while the outer regions gradually dissipate, implying a smooth transition in stellar density from the core outwards.
