The galaxy presents a primarily smooth morphology, with a high degree of central concentration. There is little evidence of a distinct spiral structure. The light profile appears relatively diffuse toward the outer regions, transitioning to a more intense, yellowish hue toward the center. This color gradient suggests a possible difference in stellar populations or dust content between the core and the outer regions. The overall shape is close to being round, with only a subtle deviation from perfect circularity. There appears to be minimal sign of significant recent or ongoing mergers or tidal disturbances. Minor disturbances may be present but no major mergers are seen.
