The galaxy presents a prominent, centrally located bulge, exhibiting a concentrated luminosity profile suggestive of an older stellar population. Emerging from the bulge, a disk structure is visible, exhibiting a grand design spiral morphology. Two well-defined spiral arms can be traced, displaying a moderate winding pattern. Patches of bluer luminosity, indicative of ongoing star formation, are sparsely distributed within the spiral arms. No significant dust lanes are discernible. There is no apparent bar feature bisecting the bulge. The overall structure indicates minimal disturbances from interactions with neighboring galaxies. The galaxy exhibits a redshift consistent with a cosmologically significant distance.
