The galaxy appears to be a spiral galaxy, observed nearly edge-on. A prominent central bulge is visible, displaying a yellowish-orange hue, suggesting an older stellar population. The disk of the galaxy is elongated and thin, extending outwards from the bulge. The outer regions of the disk show bluer tints which indicates younger, hotter stars. Dust lanes appear to be present within the disk, although not sharply defined. There is no strong indication of a recent major merger event or significant tidal distortion. The overall color suggests intermediate star formation activity. The bulge appears to be primarily rounded in morphology. There is no obvious bar structure.
