The galaxy presents a generally smooth, elliptical morphology. A bright, concentrated central bulge dominates the galaxy's luminosity profile. The light appears relatively uniform, showing a subtle color gradient from a yellower center to a slightly bluer periphery, suggesting older stellar populations concentrated in the core and possibly some younger stars in the outer regions, though active star formation is not readily apparent. There is no clear evidence of spiral arms or a distinct disk structure. The overall structure suggests a relatively relaxed system with no indications of recent major mergers or significant tidal disturbances. It appears as a well-defined, rounded shape with a high degree of symmetry.
