The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology. It exhibits a gradual radial decrease in luminosity, lacking any distinct spiral arm structure or bar features within the limits of image resolution. Color gradients are subtle, with a slightly yellower central region transitioning to bluer outskirts. There is no obvious evidence of recent or ongoing major merger activity or significant tidal disturbances affecting the overall structure. The galaxy appears largely undisturbed.
