The galaxy presents as a spiral type, exhibiting a disk-like morphology. The disk is not viewed edge-on but rather at a slight angle relative to our line of sight. There appears to be ongoing or recent interaction or merger activity, producing a somewhat disturbed appearance with asymmetries in the disk. Faint spiral arm structures are discernible, with at least two arms identifiable. The winding of these arms appears to be of medium to loose pitch. While there isn't a prominent bulge, a central region of increased light concentration is observed, suggestive of a moderate to small sized bulge component. Evidence of a bar is present although not particularly strong. The overall light distribution shows a strong presence of blue light, indicating a high fraction of young, hot stars and active star formation regions.
