This galaxy presents as a centrally concentrated object with an overall elliptical morphology. The core region exhibits a distinct yellowish-orange hue, indicative of an older stellar population. Moving outward from the core, there is a transition towards a bluish halo or disk-like structure, possibly suggesting a region of more recent or ongoing star formation. The galaxy appears to be relatively smooth, with no immediately obvious signs of strong spiral arm structures or major disturbances. The object appears more elongated than circular. There are no visible signs of a major ongoing merger or strong tidal interactions. The overall appearance is consistent with an early-type spiral galaxy or a lenticular galaxy transitioning away from active star formation in the core.
