The galaxy presents as a relatively smooth, elliptical-like object. It exhibits a concentrated central bulge that appears luminous, suggesting a high density of stars in the core. The outer regions of the galaxy fade gently into the background, showing a decrease in stellar density with increasing radius. The overall color appears somewhat redder, indicating an older stellar population. There's no obvious presence of spiral arms or significant dust lanes. The galaxy appears to be relatively undisturbed, showing little evidence of recent major merger activity. It does not show any distinct features to suggest a barred spiral structure. The apparent lack of blue light suggests a low star formation rate.
