The galaxy appears as a moderately concentrated, slightly elongated, diffuse object. Its color is generally reddish-orange, suggesting an older stellar population or significant dust obscuration. There may be a faint tidal feature or minor disturbance extending from the primary body of the galaxy, indicating a possible past interaction or merger event. The morphology is likely an elliptical galaxy exhibiting characteristics of a minor merger. The galaxy's estimated half-light radius indicates it is a large, luminous galaxy, with a high mass. The suppressed star formation rate suggests it is a red and dead galaxy that is not actively forming stars.
