The galaxy appears to be a lenticular or early-type spiral galaxy, viewed at a moderate inclination. It exhibits a prominent central bulge that dominates its overall luminosity. The bulge appears smooth and featureless with an orange hue, suggesting an older stellar population. A faint, flattened disk extends outwards from the bulge. The disk shows subtle hints of spiral structure, although it is not well-defined, along with faint blue star formation regions. The galaxy displays a color gradient, transitioning from the central orange bulge to a bluer, outer disk. There is no evidence of a major ongoing merger or strong tidal disturbances. The galaxy appears relatively isolated and undisturbed.
