The galaxy presents as an elliptical or lenticular type. It exhibits a relatively smooth, centrally concentrated light profile, lacking prominent spiral arms or significant dust lanes. The color gradient suggests an older stellar population, trending towards redder hues, particularly within the core. The morphology appears largely undisturbed, showing no signs of major mergers or tidal interactions. Its rounded shape is indicative of minimal rotational support. There is a faint, diffuse halo surrounding the bright central region. The object is relatively compact, with a gradual decrease in luminosity from the center outwards.
