The galaxy presents as a singular, relatively smooth structure, demonstrating a high degree of central concentration. There is no discernible spiral arm structure or obvious disk component. The light profile appears largely elliptical. The galaxy exhibits a color gradient, transitioning from a brighter, yellower core to a fainter, redder halo, suggesting an older stellar population dominates the galaxy's composition. There is no evidence of significant ongoing star formation activity based on the color and morphology. Overall, the galaxy appears to be a relatively quiescent system.
