The galaxy appears to be a spiral galaxy, observed at a near face-on orientation. The spiral arms are tightly wound around a bright, concentrated central bulge. The bulge is relatively small in comparison to the overall galactic disk. The spiral arms exhibit a flocculent structure, with numerous star-forming regions visible as bluish concentrations within the arms. The dust lanes are not particularly prominent. The disk appears largely undisturbed, with no major signs of tidal interactions or significant morphological distortions. The overall color of the galaxy suggests ongoing star formation, though with a relatively low star formation rate and high specific star formation rate. It shows multiple spiral arms. A possible bar structure is present, though it is not strongly defined.
