The galaxy appears to be a spiral type, with a notable disk structure. The orientation of the galaxy presents an edge-on or nearly edge-on profile. Two distinct spiral arms are visible, loosely wound and extending outward from the galactic center. There is evidence of a central bar structure spanning roughly across the galaxy's core. The bulge is likely small to moderate in size relative to the overall disk. Star formation seems to be occurring within the spiral arms, as indicated by their relatively blue hue. The general shape is not smooth, exhibiting features associated with spiral structures. There are no strong indications of major merging events or significant tidal disturbances, although minor disturbances cannot be ruled out.
