The galaxy appears to be a relatively smooth and centrally concentrated system. Its overall morphology suggests an elliptical or lenticular type. The central region exhibits a bright, yellowish-orange color, indicating a population of older stars. The outer regions become progressively fainter and redder, suggesting a decrease in stellar density and a possible difference in stellar populations, with either older stars or more dust obscuration in the outer parts. There is little evidence of distinct spiral arms or active star formation regions from the image alone. The galaxy's profile appears mostly rounded with a mild ellipticity. There is no visible evidence of major ongoing mergers or significant tidal disturbances in this image.
