The galaxy presents as a relatively smooth, centralized object with a generally elliptical morphology. There is a slight elongation noticeable, but it is largely round. A core is visible, with a slightly brighter concentration toward the center, indicating possible increased density. The galaxy exhibits color variation, suggesting differing stellar populations and activity across its structure, possibly with subtle indications of past minor disturbances but otherwise showing little or no signs of merging or tidal disruption. 
