The galaxy appears to be a spiral galaxy at an approximate redshift of 0.189, which is approximately 2.6 billion light-years away. A rough calculation suggests that the half-light radius is approximately 6 kpc. 

The galaxy exhibits a bright, moderately sized bulge, with no indications of being particularly dominant. Evidence of a bar structure is present, with a suggestion of a moderate bar. Prominent spiral arms are visible, which appear loosely wound. There is no obvious sign of any major disturbances or mergers.

The color gradients suggest a mix of stellar populations, with the bulge exhibiting more yellow tones and the spiral arms showing bluer colors indicative of ongoing star formation. The galaxy shows a low star-forming rate, suggesting a relatively quiescent period of stellar birth. The overall morphology suggests a mature galaxy.