The galaxy presents as an elongated, disk-like structure, oriented approximately along the horizontal axis in this image. A prominent central bulge dominates the galaxy's luminosity profile, appearing bright and somewhat unresolved. This bulge exhibits a slightly reddish-yellow hue, suggesting an older stellar population.

Extending outward from the bulge is a faint, bluish disk component, visible on either side. The disk shows only subtle hints of spiral structure. The blue color suggests the presence of younger, hotter stars associated with ongoing, albeit potentially low, star formation. The overall impression is that the galaxy is likely a late-type spiral or possibly an early-type lenticular, with a smooth and relatively featureless disk compared to grand design spirals. There is a slight asymmetry in color between the sides of the galaxy, possibly due to uneven dust distribution or variations in stellar population age. No signs of significant tidal disturbances or ongoing mergers are apparent.
