The galaxy presents a roughly elliptical morphology with a notable concentration of light towards the center. The central region exhibits a yellowish hue, suggesting an older stellar population dominating the core. Surrounding the core, a diffuse, less luminous halo is observed. The halo appears smoother in texture, with a gradual fade in intensity towards the outer edges. There are faint hints of a disk-like structure, but no well-defined spiral arms or strong morphological features are discernible. Overall, the galaxy appears to be a relatively quiescent system, with no significant signs of active star formation or major disturbances. The color gradients suggest a possible radial age distribution of the stars, with older populations concentrated towards the center and potentially younger populations distributed more peripherally. There may be evidence of a minor interaction or past merger event, based on asymmetries, but the general structure suggests that the system is relatively relaxed and well-mixed.
