The galaxy presents a largely smooth, elliptical morphology. It appears approximately round in shape, with only a slight deviation from perfect circularity. Its light profile is concentrated towards the center, with a gradual decrease in intensity moving outwards. There is some indication of minor disturbances, possibly suggestive of past or ongoing interactions, but no major mergers or disruptions are readily apparent. Color gradients are visible across the galaxy, transitioning from a yellowish core, possibly indicating an older stellar population, to a redder halo. Overall, the galaxy shows characteristics of a massive system with limited current star formation.
