The galaxy appears to be an elliptical galaxy, with a smooth, spheroidal shape and little evidence of spiral arms or a disk structure. The central bulge is bright and concentrated, exhibiting a yellowish hue, suggesting a population of older stars. There is a gradual decrease in luminosity moving outward from the core, with the outer regions appearing more diffuse and less distinct. There is a hint of bluer tones in the outer edges, but they seem to be extremely faint. Overall, the galaxy displays high symmetry. No obvious signs of tidal disturbances or merging features are present. The overall color suggests a relatively low rate of star formation.
