The galaxy presents as a largely smooth, elliptical morphology with a slight elongation. Its color profile exhibits a central concentration of yellow light, transitioning to a greenish-blue hue in the outer regions. There may be minor disturbances in the galaxy’s structure. The light distribution suggests a centrally concentrated stellar population with some evidence of ongoing, albeit low-level, star formation in the outer regions. The galaxy appears relatively isolated, showing no obvious signs of recent major merger activity, though some minor disturbances may be present.
