This galaxy presents as a spiral type, possessing discernible spiral arm structures. These arms appear somewhat flocculent, displaying a patchy distribution of stellar populations and dust. The galaxy exhibits a prominent central bulge, though it does not appear to dominate the overall galactic structure. The bulge's color is noticeably yellower compared to the disk, indicative of an older stellar population. The disk shows a bluer hue, suggesting ongoing star formation. Evidence of a weak bar structure is potentially present, though the resolution limits certainty. There is no obvious sign of significant ongoing merger activity or major disturbances, although some minor irregularities in the disk's morphology hint at possible past interactions. The galaxy is not seen edge-on. The overall morphology suggests a galaxy in a relatively quiescent state, with moderate star formation activity concentrated within its spiral arms.
