This galaxy presents as a spiral, inclined relative to our line of sight, displaying a clear disk-like structure. It appears to possess well-defined spiral arms, although these are somewhat flocculent and not tightly wound. A prominent, elongated central bar structure is observed, spanning a significant fraction of the galactic diameter. The bulge appears relatively small to moderate in size compared to the overall disk. The disk exhibits a degree of patchiness, suggesting active star formation regions interspersed throughout. The galaxy does not appear to be undergoing any major merging events or significant tidal disturbances, though minor disturbances cannot be ruled out. The galaxy shows a bluer color in the disk regions compared to the bulge, indicative of ongoing star formation.
