The galaxy presents a largely smooth morphology, with little discernible structure such as spiral arms or a prominent bar. It appears elliptical in shape, exhibiting a high degree of central concentration. The light profile suggests a relatively uniform stellar population. There is a color gradient visible, transitioning from a yellowish-white core to a slightly bluer halo. The halo shows a smooth falloff in luminosity, fading gradually into the background sky. There is no obvious evidence of significant tidal disturbances or ongoing major mergers. Subtle irregularities within the smooth profile cannot be ruled out.
