The galaxy appears to be an elliptical type, exhibiting a smooth, centrally concentrated morphology with no prominent spiral arms or distinct disk structure visible. The light profile suggests a relatively uniform stellar population with a slight color gradient, possibly indicating older stars are concentrated towards the core. The object has an overall rounded shape. There is a subtle asymmetry or possible minor disturbance in the galactic halo, perhaps caused by a minor merger event or tidal interaction. There is some light in the blue and yellow areas, meaning that there is on-going star formation. Overall, the object appears to be a relatively undisturbed, mature system.
