The galaxy presents a prominent, moderately sized bulge, suggesting the presence of an intermediate-mass supermassive black hole at its center. The bulge appears yellowish, indicative of an older stellar population. Extending from the bulge, we observe flocculent spiral arms. These arms appear somewhat patchy and not as tightly wound, indicating that the galaxy is likely undergoing active, but not highly organized, star formation. There is a hint of a bar structure, although not very pronounced. The galaxy shows no obvious signs of major mergers, although there may be minor tidal disturbances. The galaxy appears to be a typical spiral galaxy at a redshift of approximately 0.2, showing a disk dominated morphology.
