The galaxy presents as a roughly elliptical structure, with a dominant, concentrated central bulge exhibiting a yellowish hue. The outer regions display a more diffuse, bluish tint, suggesting the presence of a younger stellar population relative to the core. While the galaxy is generally smooth in appearance, there are subtle irregularities and hints of disturbed structure particularly in the outer regions, possibly indicating past or ongoing interactions with a smaller companion galaxy. The overall color gradient from yellow to blue suggests a radial variation in stellar populations, potentially indicative of inside-out galaxy formation or differential quenching of star formation across the galactic disk.
