The galaxy presents as an edge-on spiral galaxy, with a prominent, relatively large, and rounded central bulge. The disk component appears thin and elongated. The bulge exhibits a yellowish-orange hue, suggesting an older stellar population. The disk shows some bluer regions particularly near the edges, hinting at ongoing star formation. The galaxy displays no obvious signs of major mergers or strong tidal disturbances. The disk appears smooth. It is estimated to have significant stellar mass and moderate star formation activity.
