The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high degree of concentration, appearing bright and yellowish-white in color, indicative of an older stellar population. The outer regions gradually fade in intensity, displaying subtle color variations with hints of redder hues. The overall shape approximates roundness, with no apparent spiral arm structures or significant disturbances. There is no evidence of a major ongoing merger event, though subtle asymmetries or faint tidal features may be present upon closer inspection. The galaxy likely represents a relatively massive system, undergoing a relatively low rate of star formation.
