The galaxy exhibits a smooth, elliptical morphology with a high degree of central concentration. There is no apparent spiral structure or prominent disk features. The light profile appears diffuse, indicating a significant spheroid component. The galaxy appears to be slightly elongated. The color gradient shows a general trend toward bluer colors in the outer regions compared to the core, which exhibits a yellower hue. This may indicate ongoing or recent star formation in the outskirts of the galaxy with potentially older stellar populations towards the center. There are no indications of any major mergers or tidal disturbances.
