The galaxy presents as a disk galaxy seen nearly edge-on. A central bulge is evident, appearing with a rounded morphology and a yellowish hue, suggesting an older stellar population. The disk appears significantly flattened and elongated, with a bluer color gradient extending away from the bulge, indicative of ongoing or recent star formation. There is no evidence of major mergers or significant tidal disturbances. The disk is relatively smooth and the galaxy as a whole has an approximate mass of 10^10 solar masses, with moderate star formation activity for its mass.
