The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. It exhibits a dominant yellowish-orange hue, suggesting a population of older stars. There is little evidence of spiral arm structure or significant dust lanes within the visible portion of the galaxy. The overall light distribution is relatively even, indicating a well-mixed stellar population. The shape is approximately circular. There is no obvious presence of tidal tails or other signs of recent major merger activity. The light is fairly compact, suggesting a dense and massive system.