The galaxy exhibits a distinct spiral structure, characterized by two prominent arms emanating from a central bulge. The spiral arms appear moderately wound and extend outwards, displaying a degree of fragmentation. The central bulge appears moderate in size compared to the overall galactic disc, displaying a fairly compact appearance. The overall color profile suggests active star formation within the spiral arms and a somewhat older stellar population within the bulge. There appears to be minor disturbances to the disk. No strong bar structure is discernible within the central region. The galaxy's morphology suggests an intermediate stage of evolution, displaying characteristics of both active star formation and a developed bulge component. 
