This galaxy exhibits a primarily elliptical morphology, appearing largely smooth and lacking prominent spiral arm structures. The light distribution suggests a concentration of older stellar populations toward the galactic center, evidenced by the yellow-red hue of the core. The outer regions show a gradual decrease in surface brightness, with a slightly bluer tint, potentially indicating the presence of younger stars in these areas. The overall shape is moderately elliptical, with an axis ratio that suggests a mild flattening. There are no immediately obvious signs of major disturbances from mergers or tidal interactions, but the presence of minor irregularities cannot be ruled out without further analysis.
