The galaxy appears to be an elliptical galaxy, exhibiting a smooth, relatively featureless morphology. Its light distribution is concentrated towards the center, with a gradual decrease in brightness towards the outer regions. The galaxy displays a near-spherical shape. There are no obvious signs of spiral arms or a prominent disk structure. The galaxy does not appear to be undergoing a major merger or strong tidal interactions, though there might be slight disturbances in the outer regions indicating minor disturbances. The overall color suggests a stellar population that is dominated by older stars, indicating a low star formation rate.
