The galaxy appears as a centrally concentrated, moderately luminous object. The overall morphology suggests an elliptical or lenticular form, displaying a smooth, featureless structure with no apparent spiral arms or significant dust lanes. The core region exhibits a yellowish hue, possibly indicating an older stellar population. Moving outward, the galaxy displays a gradient toward slightly bluer colors, potentially indicating the presence of some younger stars. The outer regions appear less defined, fading gradually into the background sky. There is no discernible major disturbance, and the overall structure seems relatively relaxed and unperturbed.
