The observed galaxy exhibits a complex morphology, appearing to be undergoing a significant interaction or merger. There is evidence of disturbance in the galaxy's overall structure, with no clearly defined spiral arms or elliptical shape readily discernible. The galaxy's central region displays a relatively smooth appearance. Off center, there are two distinct bright regions that are seen. The galaxy has an overall circular shape. The color distribution shows a presence of redder hues in one of the off center regions and a bluer hue in the other off center regions. These differences in color suggest variations in stellar populations and possibly ongoing star formation in the bluer region.
