The galaxy presents an overall elliptical morphology, appearing largely smooth with a possible faint disk-like structure. It displays a centrally concentrated bright nucleus. There are some hints of bluer hues in the outer regions, suggestive of ongoing star formation, although the overall color profile is somewhat redder. The shape seems to be slightly elongated, not perfectly circular. There is no strong visual evidence of major mergers or significant tidal disturbances; however, minor perturbations cannot be ruled out.
