The galaxy presents a generally smooth, elliptical morphology. Its shape is primarily in between elliptical and spherical, with a high concentration of light towards the center. A subtle disk component cannot be ruled out. There is no apparent evidence of ongoing major mergers or strong tidal disturbances, though some minor disturbances might be present. The overall color profile suggests a mix of stellar populations, with a slight trend toward older, redder stars dominating the light output. Given its estimated size and luminosity, it appears to be a moderately massive galaxy with moderate star formation properties, but dominated by more evolved stars.
