The galaxy presents as a relatively smooth, elliptical or spheroidal structure. Its color is predominantly reddish-yellow, suggesting an older stellar population with a lower rate of star formation. There is no discernible spiral arm structure or prominent dust lanes. The overall morphology suggests a galaxy that is either a relatively undisturbed elliptical or a late-stage spiral that has exhausted much of its gas and dust. It exhibits a high degree of roundness in its shape, with no significant tidal disturbances or signs of ongoing merger activity. The color gradient appears to be consistent across the galaxy, indicative of a well-mixed stellar population.
