The object presents as a galaxy with a generally smooth, elliptical morphology. The light distribution appears highly concentrated towards the center, exhibiting a bright, well-defined core. The color gradient shifts subtly from a yellow-white central region to a more reddish hue in the outer regions, suggesting a stellar population gradient with potentially older, redder stars dominating the outskirts. There is no prominent spiral structure or significant dust lane apparent in this imagery. The object has a high degree of circularity with minimal disturbances, suggesting a relatively relaxed dynamical state. 
