The galaxy presents as a relatively faint, elongated structure. It appears to be a spiral galaxy, although the spiral arms are not sharply defined. The morphology suggests a disk-like structure seen at a high inclination, possibly approaching edge-on orientation. There's a slight bulge in the center, implying a concentration of older stars in the nucleus. The color profile suggests active star formation, albeit at moderate levels. The galaxy appears to be isolated, with no obvious signs of recent or ongoing mergers. The overall light distribution implies a considerable mass, indicative of a mature galaxy, likely experiencing normal evolution for its type and redshift.
