The galaxy appears as a lenticular-like system, possibly of type S0. It exhibits a bright, centrally concentrated bulge that transitions smoothly into a fainter, more diffuse disk. The bulge exhibits a yellow-white hue, suggesting an older stellar population. The surrounding disk shows a slight blue tint, implying the presence of some younger, hotter stars, though overall star formation activity seems to be minimal. The disk has a relatively smooth texture. The galaxy appears relatively undisturbed.
