The galaxy presents an elliptical morphology, appearing elongated with a high degree of axial ratio. The light profile exhibits a smooth and centrally concentrated distribution, indicative of a lack of significant spiral arm structures. Color gradients suggest that the core region is dominated by older stellar populations, displaying a yellowish hue. The outer regions are less well-defined but show hints of bluer colors. The galaxy displays no obvious signs of major mergers or tidal disturbances.
