The galaxy presents as an elongated, edge-on disk galaxy. The central bulge is a smooth, concentrated region exhibiting a yellowish-white hue, suggesting an older stellar population. This bulge appears predominantly rounded with a likely absence of significant recent star formation. The surrounding disk is observed nearly edge-on, characterized by a slightly bluer tint than the bulge, hinting at ongoing or recent star formation within the disk. Overall, the galaxy's morphology suggests a relatively undisturbed structure with no apparent signs of major mergers or significant tidal interactions. There appears to be minimal dust or gas obscuration along the disk.
