The galaxy presents a generally smooth, elliptical morphology. Its core exhibits a strong concentration of light, appearing a bright yellow-white. The intensity decreases gradually moving outward from the center, transitioning to a more diffuse halo. The galaxy displays a slight elongation, appearing more "in between" round and cigar-shaped. There is a faint disk visible. Overall, the structure does not appear to be significantly disturbed, with a reasonable amount of symmetry. The color gradients suggest an older stellar population, with little evidence of ongoing star formation. The galaxy is likely quite massive.
