The galaxy appears as a largely featureless, elliptical or lenticular structure. The central region exhibits a high degree of luminosity, indicating a concentrated distribution of stars. A slight elongation is visible, suggesting a departure from perfect sphericity. The overall color profile is relatively uniform and skewed toward the blue end of the spectrum. There is no discernible spiral arm structure or dust lane activity apparent in the image. Faint gradients in the outer regions show a gradual decline in surface brightness.
