The galaxy presents a relatively smooth and elliptical morphology. There appears to be a central bulge that dominates the galaxy's structure and exhibits a bright, concentrated luminosity. The color profile indicates a predominantly older stellar population with a slight gradient toward bluer hues in the outer regions. The galaxy's outer regions are slightly extended, fading gradually into the background sky. There are no obvious signs of spiral arms or prominent dust lanes. Its overall appearance suggests a relatively evolved system.
