The galaxy presents an overall elliptical morphology, exhibiting a relatively smooth and concentrated light distribution. The central region appears more luminous with a yellowish hue, potentially indicating an older stellar population. Moving outward from the core, there is a subtle shift in color, displaying a faint bluish tinge in the surrounding halo. This could suggest the presence of a younger, though still limited, stellar population within the outer regions. The galaxy shows a slight elongation, with the light distribution being more extended along one axis. There are hints of minor disturbances in its morphology, such as subtle asymmetries, suggesting possible recent or ongoing interactions. However, the overall structure remains relatively undisturbed, indicating that these interactions are not significantly disruptive.
