The galaxy presents as a largely smooth, elliptical form with a high degree of roundness. There is no discernible disk structure or spiral arm features visible in this image. The light distribution appears relatively uniform across the galaxy, lacking any bright knots of star formation or strong dust lane obscuration. There is a slight color gradient, shifting towards redder hues in the central region. Overall, the galaxy exhibits a relaxed morphology, suggesting an evolved stellar population and minimal ongoing star formation activity. There are no visual signs of recent merger events or major disturbances. The galaxy appears as an isolated system.
