The galaxy presents a generally smooth and elliptical morphology. Its light profile appears centrally concentrated, with a luminous core that gradually fades into the surrounding halo. The galaxy exhibits a color gradient, transitioning from a reddish-yellow hue in the center to a bluer tint in the outer regions. There is no apparent spiral structure or distinct disk visible in this image. The galaxy appears relatively undisturbed, with no evidence of ongoing major mergers or tidal interactions. The overall shape is somewhere between round and elliptical. Based on its color, the galaxy likely contains a mix of stellar populations, with older stars concentrated in the center and younger stars in the periphery, suggesting ongoing, but low, star formation.
