The galaxy appears as a flattened, disk-shaped structure, viewed at a high inclination, approaching edge-on. A central bulge is visible, exhibiting a smoother texture and a slightly reddish hue, potentially indicative of an older stellar population. The disk shows evidence of spiral arm structure, although they are not clearly defined; rather, a general bluer color can be seen along the edges of the disk, suggestive of ongoing star formation. This blue color might be indicative of younger, hotter stars. Dust lanes appear present, obscuring some of the starlight, particularly along the galaxy's midplane. There are no obvious signs of significant tidal disturbances or ongoing major mergers. The galaxy's morphology is primarily that of a disk galaxy, possibly a late-type spiral.
