The galaxy presents as a relatively smooth, elongated object. The primary color is a yellowish-white, suggesting an older stellar population. There is a slight color gradient with a redder hue towards the center and bluer towards the edges. This could indicate recent star formation in the outer regions, or the influence of dust. The light distribution is centrally concentrated, fading gradually towards the edges. The galaxy does not display any prominent spiral arm structures or a well-defined disk. No obvious signs of a major ongoing merger or significant tidal disturbances are present.
