The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a largely elliptical morphology. The color gradient suggests a concentration of older stellar populations towards the galactic center, with a yellow-orange hue dominating the core. Fainter, bluer hues appear in the outer regions. There is no obvious evidence of spiral arm structure or a prominent disk. The system is well-defined with no major signs of tidal disturbances or ongoing mergers. It is largely undisturbed.
