The galaxy presents as a centrally concentrated, relatively smooth object, likely an elliptical galaxy or a lenticular galaxy seen at a significant distance. The color is generally yellowish-red, indicating an older stellar population with minimal ongoing star formation, possibly containing some dust obscuration. No spiral arm structures or distinct features are immediately apparent, indicating a lack of significant disk component. The light appears to be concentrated toward the center, suggesting the presence of a bulge or a bright galactic nucleus. The general morphology suggests a galaxy that has undergone significant evolution, potentially through mergers or other processes that have disrupted any previous disk or spiral structure. The shape is generally round, showing no clear signs of disturbance from interactions with other galaxies.
