The galaxy presents as an elliptical morphology, with a smooth, diffuse appearance and no obvious spiral arm structure. It exhibits a pronounced central bulge that is significantly brighter and more concentrated than the outer regions. The color gradient suggests a stellar population that is older and redder in the central bulge, transitioning to slightly bluer hues in the outer regions. This is consistent with ongoing, though relatively low, levels of star formation in the disk component. The overall shape is elongated, indicating a substantial ellipticity; however, the isophotes appear regular and undisturbed, with no signs of major mergers or tidal distortions. The estimated size suggests a moderate physical extent.
