The galaxy appears as a relatively smooth and rounded object. It exhibits a concentrated central region with decreasing luminosity outwards. There is a slight elongation of the shape, but it is generally quite circular. A colour gradient is visible, shifting from a warmer, reddish-yellow hue in the core to a cooler, greenish-yellow at the outer edges. The smooth morphology suggests a system with minimal ongoing star formation. Faint disturbed features indicate the possibility of minor interactions with a merger in its past. The system displays what appears to be two central concentrations within the same galactic halo.
