The galaxy presents a notable disk-like structure, with a prominent central bulge region. Evident spiral arm features emanate from the core, displaying a moderately flocculent morphology. The galaxy exhibits an overall blue color, indicative of relatively recent and ongoing star formation activity. The central bulge appears comparatively brighter than the surrounding disk, suggesting a higher concentration of older stellar populations in that region. There appears to be some slight asymmetry in the distribution of light within the disk, hinting at possible minor gravitational interactions or internal disturbances. A bar structure is not immediately apparent upon visual inspection, however, this assessment might need spectral evidence.
