The galaxy presents a largely smooth and symmetrical appearance, suggesting an elliptical morphology or a disk galaxy viewed face-on. The light distribution is concentrated towards the center, with a gradual decline in brightness towards the outer regions. There is a suggestion of a yellow or orange hue, with subtle color variations across the galaxy. The light is somewhat redder in the core, implying an older stellar population or significant dust extinction. There is no evidence of spiral arms or a distinct disk. The overall structure is consistent with an evolved system undergoing little current star formation. It appears relatively undisturbed, lacking prominent tidal features or signs of a recent merger.
