The galaxy appears to be an elliptical galaxy at a considerable distance. It exhibits a smooth, centrally concentrated light distribution, with no discernible spiral arms or prominent disk features. The galaxy's core presents a yellowish hue, which suggests an older stellar population. The outer regions of the galaxy fade gradually, showing a decrease in stellar density and a slight shift toward redder colors. There is no apparent evidence of ongoing major mergers or significant tidal disturbances in this galaxy. It appears relatively undisturbed, maintaining a regular, somewhat elongated shape.
