The galaxy presents as a spiral type, with a relatively bright central bulge. Spiral arms are clearly visible, extending from the core region. These arms appear somewhat tightly wound. The galaxy is not seen edge-on; its disk is considerably inclined towards our line of sight. The bulge presents a moderate size in relation to the disk, with a yellow, red hue in the center. There is a slight blue tint in the arms of this galaxy. Based on its disturbed morphology, the galaxy shows signs of possibly undergoing a merger or significant gravitational interaction, resulting in a highly asymmetric structure. There is a possible tidal tail present as well.
