This galaxy presents as a generally smooth, elliptical-like structure. The central region exhibits a distinct concentration of light, suggestive of a prominent galactic nucleus. The color profile reveals a redder core, transitioning to a bluer halo. This color gradient could indicate an older stellar population dominating the core, with younger, bluer stars more prevalent in the outer regions. No distinct spiral arm structures are visible. There are no signs of major disturbances or ongoing mergers. The overall morphology suggests a mature galaxy with relatively quiescent star formation activity, potentially with ongoing star formation in the outer region of the galaxy. 
