The galaxy appears to be a spiral type, although its features are somewhat disturbed. There is a discernible disk structure but without a clear, grand design. Faint spiral arms are visible, with patchy regions of star formation that exhibit a bluish tint. The central bulge is small and not very pronounced. The galaxy's overall shape is irregular, potentially indicative of an ongoing or recent interaction or merger. The light distribution is uneven, suggesting that the galaxy may be undergoing active star formation or has recently experienced a burst of star formation activity. Some degree of tidal disturbance is observed, as the arms are asymmetrical.