The galaxy presents a largely smooth and centrally concentrated morphology, indicative of an elliptical galaxy. The color profile suggests an older stellar population, with a dominant yellowish hue in the central region. There is some subtle color variation extending outwards. No significant spiral arm structures or prominent dust lanes are observed. The galaxy appears relatively isolated, with no obvious signs of major interactions or mergers with other galaxies. A moderate amount of star formation may be present, but no prominent star forming regions are apparent in this image.
