The galaxy appears to be a spiral galaxy at a redshift of approximately 0.192. It exhibits a distinct disk structure, with a moderate bulge component. Faint spiral arms are visible, appearing to extend outwards from the central bulge. The winding of these arms seems to range from somewhat loose to moderately tight. There is no strong evidence of a bar-like structure. The galaxy does not appear to be undergoing a major merger, though there is some evidence of minor disturbances in the structure. The overall color suggests the presence of a mix of stellar populations, including regions of active star formation indicated by blue hues, and older stellar populations in the bulge indicated by yellower and reddish hues. The galaxy appears to have an inclination that is not edge-on.
