The galaxy presents as a spiral type, with distinct spiral arms emanating from a central bulge. The arms appear somewhat loosely wound, extending outwards from the core. There is evidence of a bar structure across the center, though it appears relatively weak. The galaxy is not perfectly face-on; it has a slight inclination which allows a view of its disk structure. The bulge is moderate in size relative to the disk. Star formation is evident within the spiral arms, as indicated by areas of bluer hue. There are some areas of redder hue as well. Overall, the galaxy seems largely undisturbed, not showing signs of a major merger.
