The galaxy appears to be a late-type spiral, exhibiting a prominent disk structure. The spiral arms are loosely wound and show evidence of active star formation, indicated by the presence of blue-tinged regions. The central bulge is relatively small, with a somewhat yellowish hue, possibly suggesting an older stellar population compared to the arms. There seems to be a tidal tail structure, hinting at a gravitational interaction with another galaxy. The galaxy exhibits irregular features, especially distortions and asymmetries, which would be consistent with an ongoing or recent merger event. The overall color index suggests a relatively high star formation rate within the galaxy. 
