The galaxy presents as a relatively smooth, elliptical-like structure. The central bulge exhibits a concentrated luminosity, with a gradual decrease in surface brightness toward the outer edges. There is a subtle color gradient visible, with a slightly yellower hue towards the center and a bluer tinge in the outer regions. This suggests a potential difference in stellar populations, with older, redder stars dominating the core and younger, bluer stars in the surrounding areas. The overall shape appears close to round, with minimal signs of significant tidal disturbances or ongoing major mergers. Faint hints of asymmetry may indicate a past minor interaction or internal dynamical processes.
