The galaxy presents a generally smooth and elliptical morphology. Its core is a bright, concentrated yellow, suggesting a population of older stars. There is a slight reddish halo in the outskirts, which is also a sign of aging stars. The overall roundness is high and there are no distinct spiral arms or significant disturbances evident in its structure, which indicates a lack of recent major mergers. It exhibits a color gradient, with the core being more yellow than the surrounding regions. This implies a radial variation in stellar populations or dust content within the galaxy.
