The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. It exhibits a bright, compact core that diminishes in intensity with increasing radial distance. There appears to be little evidence of spiral arm structures or prominent dust lanes. The color gradient indicates a higher concentration of older stellar populations in the central region, trending towards a bluer hue in the outer regions. There is very little evidence of star formation activity within the galaxy based on its smooth texture. The overall appearance indicates a mature galaxy that has undergone significant stellar evolution. The galaxy has a roughly axisymmetric shape with only a slight distortion.
