The galaxy appears as a centrally concentrated object with a relatively smooth, featureless morphology. The light distribution suggests a dominant spheroidal component, potentially an elliptical galaxy or a lenticular galaxy seen at a shallow inclination. There is a color gradient, with a more pronounced yellow-orange hue toward the center, suggesting an older stellar population in the galactic nucleus. The outer regions exhibit a slightly bluer tint, possibly indicating the presence of younger stars, though the overall color is still indicative of a galaxy with limited ongoing star formation. The galaxy is somewhat elongated along one axis, which, in tandem with the central concentration, would mean that it is likely a galaxy lacking a prominent spiral structure.
