The galaxy presents a non-smooth morphology, exhibiting a distinct disk structure. Within the disk, spiral arm features are readily apparent. These arms display a range of winding, from medium to loose. A strong bar is not evident, but the presence of a weaker bar feature cannot be ruled out. The bulge size appears to be relatively small, indicating a lower concentration of stars in the central region compared to the disk. Possible minor disturbance, major disturbance, or merger is occurring in this system. It is likely merging with another galaxy.
