The galaxy presents a largely smooth, centrally concentrated morphology. The light distribution appears relatively uniform, lacking prominent spiral arms or bar structures. The shape is generally round. There is faint evidence of asymmetry, possibly indicating a minor disturbance or interaction, though the overall structure is dominated by a smooth, spheroid-like appearance. Color gradients suggest a potential redder core, with bluer light extending towards the outer regions. This suggests a distribution of stellar populations where older stars are more concentrated in the center.
