The galaxy presents as a spiral type, exhibiting well-defined spiral arms emanating from a central bulge. The spiral arms appear somewhat fragmented and display varying degrees of winding tightness; medium and tight winding are observed. Color variations suggest active star formation regions within the arms, with a dominant blue hue indicative of a younger stellar population. The central bulge appears moderate in size and exhibits a smoother texture compared to the arms. A faint bar-like structure may be present, extending from the central bulge. The disk is viewed close to face-on. Irregularities in the galaxy's shape and brightness distribution may suggest minor gravitational interactions or disturbances with smaller satellite galaxies. The overall structure indicates a galaxy undergoing ongoing star formation, residing at a redshift distance of 0.052181.
