The galaxy exhibits an overall elliptical morphology with a high degree of central concentration. The core region displays a yellowish-white hue, suggesting an older stellar population dominating the central bulge. Moving outward from the core, a gradual transition towards bluer colors is observed, indicating the presence of younger stars and possibly ongoing star formation in the outer regions. Faint, diffuse extensions are visible, though distinct spiral arm structures are not apparent. There are some subtle hints of possible minor disturbances in the morphology, perhaps from a past or ongoing minor merger event. However, the galaxy largely appears undisturbed with a smooth and relatively symmetric structure.
