The galaxy appears to be a relatively smooth, elliptical system. The central region exhibits a strong concentration of light, with a yellowish-orange hue, suggestive of an older stellar population. This color likely indicates a dominance of red giant stars within the core. Surrounding this central bulge is a fainter, more diffuse halo. Hints of a disk-like structure exist. There are no prominent spiral arms or other significant features. The overall symmetry suggests that the galaxy is relatively undisturbed and in a late stage of its evolution. There is a slight asymmetry to the left side. There may be ongoing minor merging activity.
