The galaxy presents as an elongated, disk-shaped structure oriented nearly edge-on to our line of sight. The central bulge is not particularly prominent, exhibiting a moderate concentration of light, with a color gradient suggesting an older stellar population dominating this region. The disk shows evidence of dust lanes, particularly along the mid-plane, which attenuates light and creates a darker band. The overall color of the galaxy is yellowish, with a hint of blue towards the outer edges of the disk, indicating the presence of some younger stars and ongoing star formation. No significant tidal features or signs of a major merger event are apparent, although some minor asymmetries within the disk could be indicative of a small interaction or internal disturbances.
