The galaxy presents as a smooth, elongated structure, likely a lenticular or edge-on spiral galaxy given its apparent shape. The central bulge appears brighter and more concentrated, exhibiting a yellowish-white hue, suggesting an older stellar population dominating this region. Fainter, bluish light is visible at the extremities of the disk, hinting at some younger, hotter stars and possible ongoing star formation in these outer regions, although the rate is likely low. The galaxy does not show any obvious signs of major mergers or significant tidal disturbances in this image, appearing relatively undisturbed.
