The observed galaxy presents as an edge-on spiral, exhibiting a flattened disk-like structure. A prominent dust lane bisects the galaxy along its major axis, obscuring the central bulge and contributing to its overall elongated appearance.

The disk displays a mottled texture, indicating the presence of star-forming regions. These regions appear as brighter, somewhat knotty areas within the disk, concentrated along spiral arm segments. The spiral arms themselves are not clearly defined, appearing somewhat flocculent.

No prominent central bulge is observable, suggesting either a small bulge or obscuration by the aforementioned dust lane. There are no obvious signs of a major merger event, although some minor distortions or asymmetries may be present within the disk structure. Light is brightest in the middle, where it appears to be slightly thicker. 

The galaxy's color suggests a population of young, hot stars within the disk, as well as older, cooler stars.
