The observed galaxy presents as a spiral galaxy, exhibiting a prominent central bulge. The bulge appears bright, suggesting a concentration of older stellar populations. Faint spiral arms emanate from the central region. The arms are not well-defined, indicating they are either tightly wound or that this is a flocculent spiral galaxy with patchy, discontinuous arm segments. 

The overall color of the galaxy is slightly blue-shifted, particularly in the disk region, hinting at ongoing star formation. There is no apparent bar structure visible in the image. The galaxy appears relatively undisturbed, with no major morphological signs of a recent merger event visible. The bulge appears moderate in size relative to the disk, which may explain the star formation observed in the image.