The galaxy appears as a largely featureless, elliptical or lenticular system. The light profile exhibits a smooth, centrally concentrated morphology with no discernible spiral arm structure or dust lanes. The color appears to be dominated by redder wavelengths, indicating an older stellar population and potentially lower levels of ongoing star formation. The galaxy appears relatively isolated with no obvious signs of recent or ongoing major merger activity. There is no discernible tidal debris or morphological disturbances in this image. The overall shape of the galaxy seems nearly circular, with no significant elongation.
