This galaxy presents as a relatively smooth, elliptical structure. The central bulge appears bright and concentrated with a yellow hue, suggesting an older stellar population. There is a gradual decrease in luminosity from the core to the outer regions. The galaxy exhibits a slight elongation, but does not appear heavily distorted or disturbed. Faint blue tinges in the outer regions may indicate some presence of younger, hotter stars, though it is not a dominant feature. Overall, the morphology suggests a relatively evolved system without prominent spiral arms or significant ongoing star formation.
