The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits a golden hue, potentially indicating an older stellar population. The galaxy appears largely undisturbed with no obvious signs of tidal interactions or mergers, based on the smooth morphology and lack of discernible features, suggesting a degree of quiescence in its recent evolutionary history. The disk is not apparent, making the classification of an elliptical galaxy more plausible.
