The galaxy presents as a spiral type, with a prominent disk structure. Spiral arms are clearly visible and appear somewhat loosely wound. One dominant spiral arm emerges from the bright center, which likely hosts an actively star-forming region. There appears to be a minor disturbance present, perhaps the result of a tidal interaction or recent minor merger. The bulge component appears moderate in size compared to the disk. There is a slight asymmetry in the disk's overall shape. The overall color of the galaxy appears to be shifted towards redder wavelengths.
