The galaxy presents a largely smooth, elliptical morphology. A bright, concentrated central bulge dominates the structure, exhibiting a strong orange hue, possibly indicating an older stellar population. The outer regions show a more diffuse and mottled texture. The overall color appears slightly redder than the core, suggestive of ongoing, albeit subdued, star formation activity within the galaxy's disk. There are no immediately obvious signs of a major merger event, but a subtle asymmetry in the outer regions could hint at a minor interaction or disturbance.
