The galaxy presents as an edge-on disk galaxy, with a prominent central bulge. The bulge appears relatively smooth and concentrated. The disk is thin and elongated. There is evidence of dust obscuration along the galactic plane, particularly noticeable in the lower half of the galaxy. Star formation appears to be present within the disk, although it is not especially vigorous. There is a lack of any major tidal disturbances or ongoing mergers visible, though a slight asymmetry within the disk structure cannot be ruled out. The light distribution suggests a well-defined, although somewhat indistinct, structure with older stellar populations concentrated in the bulge and a gradual decrease in surface brightness outwards along the disk.
