The galaxy presents as an elongated, cigar-shaped system. Its overall morphology suggests a disk galaxy viewed at a high inclination. The light distribution shows a central concentration, possibly indicating the presence of a bulge component. The disk exhibits a relatively smooth appearance, with subtle color variations along its extent. There's a hint of bluer hues in certain regions, particularly towards the edges of the disk. These bluer areas might indicate regions of younger stellar populations or active star formation. The overall color suggests a mix of stellar populations, with the brighter central region appearing more yellowish. There is no obvious grand design spiral structure visible. It appears that there are no signs of major mergers or significant tidal disturbances.
