The galaxy presents as a single, relatively smooth object with a concentrated central region. The color appears primarily yellow-orange, suggesting a population of older stars and a lower rate of on-going star formation. There is no immediately apparent spiral structure or dust lanes, indicating it could be an elliptical galaxy or a lenticular galaxy viewed face-on. The roundness is not perfectly circular, showing a slight deviation. There is no visible sign of tidal tails or other disturbances, meaning it likely is not undergoing a major merger with another galaxy, though some minor gravitational interaction cannot be ruled out. Given its size in the image and the probable distance, it seems to be a galaxy with a considerable mass.
