This galaxy appears to be a relatively smooth, elliptical or lenticular galaxy, with a slightly elongated shape. The light distribution is concentrated towards the center, with a gradual decrease in brightness outwards. It seems to be a relatively isolated system with no obvious signs of major ongoing merger activity, though there may be minor disturbances visible upon closer inspection. The galaxy displays a moderate color, suggesting a moderate amount of ongoing or recent star formation. Overall, the galaxy presents as a mature system.
