The galaxy presents as an elliptical structure, appearing generally smooth with minimal discernible features. Its shape approximates a rounded form. The light distribution exhibits a centrally concentrated profile, indicating a higher density of stars and/or gas towards the galactic nucleus. The galaxy shows a clear color gradient, trending towards bluer hues at the outskirts. This suggests an older stellar population dominating the core region, and younger stars are distributed more widely. There are no prominent spiral arms, bars, or dust lanes visible. There is no obvious tidal distortion or other signs of recent major merger activity. Given the apparent smoothness and morphology, this object is most likely classified as an elliptical galaxy. 
