The galaxy appears as a single, relatively smooth object with an elliptical morphology. There is no discernible disk structure. Its color profile suggests it's composed primarily of older stellar populations, with a bias toward redder wavelengths and less recent star formation activity. There is no apparent ongoing major merger or tidal disturbances, though minor disturbances or interactions cannot be ruled out from the image alone. The galaxy exhibits a slightly rounded appearance with axial symmetry.
