The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, with light gradually diminishing toward the outer edges. The color profile appears to be primarily yellow/orange, suggesting an older stellar population with less active star formation. There are no obvious spiral arms or dust lanes visible, which is consistent with the appearance of an elliptical galaxy. The galaxy appears isolated, lacking any immediately apparent tidal distortions or nearby companion galaxies that might indicate an ongoing or recent merger event. There is also a slight central point suggesting a central supermassive black hole. The overall morphology indicates a galaxy that has likely undergone significant evolution, resulting in a more quiescent state.
