The observed galaxy presents as an edge-on spiral or lenticular galaxy at a redshift of approximately 0.137. The galaxy exhibits a prominent central bulge, with a smooth, elliptical morphology. The bulge appears to be of the boxy type, however, it does tend to be rounded. The disk component is highly flattened and oriented nearly edge-on to our line of sight. Some dust lane obscuration is suspected along the equatorial plane, though definitive features are difficult to discern. The overall color is relatively uniform, suggesting a lack of significant active star formation. Based on its color and overall morphology, it is likely to be a fairly massive system. No signs of tidal disturbances or major mergers are apparent in this imagery, suggesting this is an isolated galaxy. 
