The galaxy presents as a relatively smooth, centrally concentrated object with a round shape. Its light profile appears consistent and lacking prominent internal structures such as spiral arms or bars. There is a subtle color gradient, with the central region appearing slightly more yellow, potentially indicating an older stellar population concentrated in the core. The outer regions exhibit a bluer hue suggesting the presence of younger stars, although this difference is not pronounced. No evidence of tidal features or significant distortions is discernible, suggesting it is not undergoing a major merger. The galaxy's overall appearance is consistent with that of an elliptical galaxy at a considerable distance, exhibiting no clear signs of ongoing, vigorous star formation.
