The galaxy appears to be a relatively smooth, lenticular or early-type spiral galaxy, likely at an advanced evolutionary stage. It exhibits a prominent bulge and a diffuse disk. The color gradient suggests a redder bulge region, indicating an older stellar population, while the disk shows a bluer hue, indicating recent or ongoing star formation at a low rate. The overall shape is elliptical but close to round, indicating that the galaxy is most likely not viewed edge-on. There is no evidence of a major merger event, although minor disturbances or tidal features may be present.
