The galaxy presents a largely smooth morphology, with a high degree of central concentration. It exhibits an elliptical shape, nearly circular, with a hint of elongation. There are no visible spiral arms or distinct features like bars or rings. The galaxy displays a color gradient, transitioning from a bluer hue at the center to a slightly redder periphery. This suggests a potential difference in stellar populations or dust content between the core and outer regions. No evidence of major disturbances, tidal tails, or ongoing mergers can be observed within the limitations of the image resolution.
