The galaxy appears to be a spiral type, presenting a disk-like structure with a discernible bulge. The spiral arms are not sharply defined, appearing somewhat flocculent. The overall color of the galaxy leans towards the blue end of the spectrum, suggestive of ongoing star formation. There is some indication of internal structure or possible minor disturbance in the disk. The object's ellipticity is moderate, with an intermediate roundness. No major merger events are readily apparent, though there might be some minor disturbances present. The object's apparent magnitude suggests moderate luminosity. 
