The galaxy presents as a smooth, elliptical-shaped structure with a noticeable central bulge. The light distribution appears relatively uniform, lacking prominent spiral arms or distinct features. A slight elongation is visible, suggesting it is not perfectly spherical. The galaxy displays a color gradient, appearing bluer in the outer regions and transitioning to a redder hue towards the core. This color difference could indicate variations in stellar populations, with younger, bluer stars populating the outskirts and older, redder stars dominating the central bulge. There are no obvious signs of ongoing major mergers or tidal disturbances within the observed field of view.
