The galaxy appears to be an elliptical type, displaying a smooth, featureless morphology with a high degree of roundness in its overall shape. The central region exhibits a bright, concentrated light profile, suggesting a significant stellar population and/or active galactic nucleus activity. The light is mostly concentrated in the center with the intensity quickly tapering towards the edge of the image. The light distribution is very uniform with no evidence of spiral arms or irregular structures. It exhibits a color gradient, appearing more yellow or orange in the core, possibly indicating an older stellar population, and transitioning to slightly bluer hues towards the periphery. There is no apparent disturbance to the morphology and the object shows no evidence of an ongoing merger.
