The galaxy appears to be a relatively smooth, elliptical galaxy with a bright central bulge. It exhibits a somewhat spheroidal shape, though there is a slight elongation visible, suggesting it is not perfectly spherical. The galaxy's light profile decreases gradually from the core outwards. No distinct spiral arms or prominent dust lanes are discernible. There appears to be very minor disturbances in the light profile, but these are not indicative of a major merger or significant interaction with another galaxy. The galaxy is likely a quiescent system with a relatively low star formation rate.
