The galaxy presents a largely disk-dominated morphology, oriented at an angle that allows for a clear view of its spiral structure. The spiral arms are well-defined and extend outwards from a central bulge. The bulge appears moderate in size. There is some visual suggestion of a bar-like structure within the central region, but the image resolution makes it difficult to assess definitively if it is a strong or weak bar. The arms show clear evidence of star formation, with the blue color suggesting the presence of young, hot stars. The overall winding of the spiral arms appears of medium tightness. Some regions of the disk exhibit disturbances, which could be attributed to minor gravitational interactions. There is no obvious evidence of a major ongoing merger or strong tidal features, but some asymmetry within the disk implies a possibility of recent interaction. 
