The galaxy presents as a somewhat elliptical, centrally concentrated light source. The core region displays a yellow-white hue, indicative of older stellar populations. There are no visible spiral arm structures or dust lanes. A faint greenish tint appears towards the edges which suggests a small amount of ongoing star formation. The galaxy appears relatively smooth and featureless, with a high degree of central concentration, and subtle gradients in surface brightness from the center outwards. There is no significant evidence of recent mergers or major disturbances in its morphology. The light is redshifted suggesting that it is relatively distant.
