This galaxy presents as an elliptical object, exhibiting a centrally concentrated luminosity profile that diminishes gradually outward. The overall shape is relatively round. There is a clear color gradient visible across the galaxy, transitioning from bluer hues in one region to redder tones in another, implying varying stellar populations or dust content. While the primary structure appears smooth, subtle asymmetries are present, hinting at the possibility of past interactions or disturbances. However, there are no obvious signs of a major merger or significant tidal features. Minor disturbances in the morphology cannot be ruled out. Overall, the galaxy appears to be in a relatively quiescent state.
