The galaxy presents as a relatively smooth, elliptical-like structure. Its color is predominantly a red-orange hue, suggesting an older stellar population with a lower rate of ongoing star formation. The galaxy appears largely undisturbed, with no significant signs of tidal features, major mergers, or strong morphological asymmetry. It exhibits a high degree of central concentration, with a smooth radial profile in luminosity. Its overall round appearance suggests a system dominated by random stellar motions rather than a well-defined rotating disk.
