The galaxy appears as a single, relatively compact object with a smooth overall morphology. The light profile suggests a moderate concentration of stars towards the center, fading towards the outer regions. The galaxy's shape appears close to round but slightly oblong, indicating a lack of a well-defined disk structure. The color suggests an older stellar population, as indicated by a redder overall hue, but with some areas of bluer light. Star formation is likely occurring at a low rate. There is no strong evidence of spiral arms or bar structures. The general morphology and color suggest a high probability of being an elliptical galaxy or perhaps a lenticular galaxy seen nearly face-on. The galaxy doesn't exhibit any clear signs of recent mergers or major disturbances, though there is a hint of a minor asymmetry in its outer regions which could suggest a past interaction.
