The galaxy presents a generally smooth and rounded morphology. Its light profile appears centrally concentrated, with a gradual decrease in surface brightness moving outward from the core. The core region exhibits a yellowish hue, suggesting a stellar population that is more evolved. The outer regions exhibit a more complex color profile, with hints of bluer patches. There may be some limited substructure visible, but overall the galaxy lacks strong spiral arms or other distinct features. The galaxy is relatively isolated and does not show clear signs of a major ongoing merger event, although the potential for minor disturbances cannot be ruled out.
