The galaxy appears to be an elliptical type, displaying a relatively smooth and featureless morphology. It exhibits a generally rounded shape, with a high degree of central concentration of light. The galaxy presents a color gradient, appearing bluer towards the outer edges and redder towards the central bulge. This color variation suggests a potential difference in stellar populations between the core and the outskirts, possibly indicating ongoing or recent star formation in the outer regions. There are hints of disturbances or tidal features, suggesting a past interaction or merger event that disrupted its original morphology.