The galaxy presents as a spiral galaxy with a moderately sized bulge. There is the suggestion of a bar feature bisecting the bulge, although the resolution is insufficient to definitively classify it as strong or weak. The spiral arms appear to be somewhat flocculent, with regions of active star formation visible as bluer patches interspersed within the arms. The disk is not perfectly face-on but shows a degree of inclination. Overall the galaxy seems relatively undisturbed, showing no signs of a major merger, though some minor irregularities in the arm structure could indicate minor gravitational interactions. The colour suggests an intermediate redshift, with both older stellar populations in the bulge visible, and ongoing star formation in the arms.
