The galaxy presents a generally smooth, elliptical morphology. The central bulge is luminous with a yellowish hue, suggesting an older stellar population. Moving outward from the core, a fainter, more diffuse disk-like structure is observed. Hints of bluer color, indicating regions of potential star formation, are subtly present in the outer regions of the galaxy. Overall, the galaxy appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions.
