The galaxy presents as a relatively face-on spiral structure. Distinct spiral arms are visible, exhibiting a slightly flocculent morphology. These arms appear asymmetric, potentially indicating past or ongoing interaction or tidal effects. There appears to be a moderately sized central bulge region. The galaxy exhibits blue hues within its spiral arms suggesting active star formation. The disk appears somewhat thin and well-defined. There might be a subtle bar-like structure present in the center of the bulge. Overall, the galaxy displays characteristics consistent with a late-type spiral morphology, with evidence of active star formation within its spiral arms. A slight visual disturbance might be present suggesting a weak gravitational interaction.