The galaxy presents a largely featureless morphology, appearing generally smooth and elliptical in shape. The light distribution suggests a centrally concentrated structure. The galaxy exhibits a dominant yellowish-orange hue, indicative of a stellar population that is likely dominated by older, redder stars, suggesting relatively low levels of ongoing star formation. The overall appearance suggests a relatively evolved system, potentially a massive elliptical galaxy. There is no visible evidence of spiral arms, dust lanes, or significant tidal disturbances.
