The galaxy appears as a centrally concentrated object, exhibiting a generally smooth morphology. The light profile suggests a relatively featureless structure. The overall shape is more rounded than elongated, appearing somewhat elliptical. There may be some minor evidence of disturbances, although the galaxy predominantly presents a unified structure. Color gradients are visible, with a core that seems slightly bluer relative to the outer regions, which show a hint of redder hues. This could indicate ongoing or recent star formation in the central regions. No signs of significant tidal tails or clear indications of recent major merger events are discernible, although a slight asymmetry cannot be entirely ruled out.
