This galaxy presents as a likely disk galaxy, viewed at an almost complete edge-on orientation. A prominent dust lane bisects the galaxy, obscuring a significant portion of the galactic plane. Some visible distortion is present, which may be indicative of a minor disturbance caused by the presence of a nearby companion galaxy or a recent merger event. Despite the edge-on presentation, some evidence of spirality can be inferred. There appears to be a large central bulge. The galaxy displays a color gradient, with the bulge appearing redder compared to the disk. The estimated half-light radius is approximately 5 kpc. Overall, the galaxy seems relatively smooth in appearance, but there is a significant amount of dust and gas. The star formation rate is relatively low.