This galaxy appears to be a spiral galaxy, exhibiting a disk-like structure with prominent spiral arms. A substantial bar feature traverses the central region, with a relatively moderate bulge size. The spiral arms are well-defined and extend outwards from the bar. There are hints of active star formation regions within the arms, evidenced by their slightly bluer color. Overall, the galaxy does not display any significant signs of a major merging event or substantial disturbances, it seems relatively isolated.
