The galaxy appears as a single, largely homogenous structure. Its color is predominantly yellow, suggesting an older stellar population, and reduced rates of star formation activity. The object presents a smooth profile with a high degree of central concentration. The morphology suggests an elliptical galaxy. It also appears to be relatively isolated, showing no indications of ongoing major mergers or significant tidal disturbances. The lack of prominent spiral arms or a well-defined disk supports the classification as an elliptical galaxy.
