The galaxy appears as a single, relatively smooth object. It exhibits an elliptical morphology, lacking any prominent spiral arm structures or a well-defined disk. The color gradient suggests an older stellar population with a redder hue dominant throughout the galaxy. There is little to no evidence of ongoing star formation activity based on the lack of blue or white regions, which are indicative of hot, young stars. The galaxy's overall structure appears undisturbed, showing no signs of major mergers or tidal distortions.
