The galaxy appears to be a relatively smooth, elliptical galaxy. It has a bright, concentrated central bulge which fades gradually into a more diffuse halo. The overall color profile suggests an older stellar population, with a yellowish hue dominating the central regions. There is no apparent dust lane or spiral arm structure visible, leading to the conclusion of a lack of substantial recent star formation. There is a slight asymmetry to the halo, but this is not enough to suspect a major merger event. The shape appears more elongated than perfectly circular, though not significantly so. There appears to be some minor disturbance, perhaps a faint tidal tail, though that is not immediately clear from the image.
