The galaxy presents as a spiral type, displaying a disk structure with relatively prominent spiral arms. These arms appear somewhat flocculent and loosely wound. There is evidence of ongoing star formation within these arms, indicated by their slightly bluer coloration relative to the rest of the disk. The galaxy exhibits a moderate central bulge, yellowish in color suggesting a population of older stars. The galaxy is observed nearly face-on, with no apparent signs of significant tidal disturbances or major mergers. There appears to be a weak bar structure. The overall appearance suggests a system with a substantial disk, active star formation in the arms, and a moderate-sized bulge.
