The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a high degree of circularity. It shows no distinct spiral arms or bar-like structure. There is a slight color gradient, appearing bluer in the core region, suggestive of some younger star formation. The outer regions appear redder, consistent with an older stellar population. The galaxy exhibits no obvious signs of ongoing major mergers or tidal disturbances, although minor asymmetries may be present. Overall, it presents the morphology of an evolved galaxy with a modest level of ongoing star formation.
