The galaxy presents a generally smooth, elliptical morphology. Its color is a blend, transitioning from a yellow-orange core to a bluish-green outer halo. This color gradient might be indicative of differing stellar populations, with older, redder stars concentrated in the core and younger, bluer stars in the outer regions. The light distribution appears largely symmetrical. Faint distortions may exist in the outer regions, potentially suggestive of past or ongoing minor interactions, although they are not prominent. Overall, the galaxy appears relatively undisturbed with no clear spiral arm structure.
