The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a high concentration of luminosity, appearing bright and somewhat yellow. The color suggests an older stellar population dominating the core. Moving outwards from the center, the luminosity gradually decreases, with a subtle transition to slightly redder hues in the outer regions. The overall shape is mostly round, though some minor distortions might be present. There appears to be no distinct spiral arm structure or prominent dust lanes. Signs of any major merger events are absent, though some minor disturbances cannot be ruled out.
