The galaxy exhibits a clear spiral structure, with prominent arms extending from a central bulge. The spiral arms display a somewhat flocculent nature, appearing patchy and less defined in certain regions. The overall color profile suggests active star formation, with blue hues concentrated along the spiral arms, indicating the presence of young, hot stars. There appears to be a moderate bulge component. The winding of the spiral arms appears to be moderately tight. Some morphological irregularity and a subtle asymmetry are apparent, possibly indicating past or ongoing minor interactions. The light is more diffuse in the outer regions, with the arms losing definition further from the bulge.
