This galaxy presents as a relatively smooth, elliptical-type system. The overall shape approximates a rounded form. The central region exhibits a concentration of light, suggesting the presence of a galactic nucleus. Fainter and more diffuse light extends outwards from the core. The color profile indicates a dominance of older stellar populations with a moderate amount of star formation activity. There is no clear evidence of significant disturbances or ongoing mergers within the system based on this image. The color is weighted slightly redder than blue.
