The galaxy presents as a spiral type, exhibiting a well-defined disk structure. The spiral arms are tightly wound around a prominent central bulge. There are most likely multiple spiral arms. The bulge appears to be of moderate size relative to the disk, with a generally smooth texture. The galaxy disk is oriented at an angle relative to the observer, allowing for observation of its spiral structure. The colour profile suggests active star formation. There does not appear to be evidence of ongoing major merger activity but there may be minor disturbances. 
