The galaxy presents as a slightly inclined disk galaxy. There's a prominent central bulge that appears yellowish-orange, suggesting an older stellar population. The disk exhibits a bluer hue, indicating the presence of younger, hotter stars and potential star formation regions. There is a hint of spiral arm structure although it is not very distinct. The disk appears relatively smooth, with no obvious large-scale disturbances or tidal features, implying it is relatively undisturbed, although some minor disturbance cannot be ruled out. Overall, the galaxy seems to be of intermediate mass with a very low star formation rate.
