The galaxy presents as a spiral type, exhibiting a disk structure with apparent spiral arms. The arms are not sharply defined, appearing somewhat flocculent. A central bulge is visible, seemingly moderate in size. The winding of the spiral arms appears to be medium to tight. There's an indication of a bar-like structure traversing the central region. The overall color profile suggests active star formation within the disk, as indicated by the bluer hues in the spiral arms. The galaxy exhibits some indication of tidal disturbances or interactions, as its shape is not perfectly symmetric, suggesting the possibility of minor or major mergers.
