The galaxy appears to be undergoing a significant interaction or merger. There are multiple distinct luminous components, suggesting the presence of at least two interacting galaxies. A central, elongated region exhibits a yellowish-orange hue, indicative of an older stellar population. Two brighter, more compact regions are present. The overall shape is irregular and disturbed, lacking the symmetry of a typical spiral or elliptical galaxy. There is possible evidence of tidal tails or bridges extending outward from the central region, further supporting the classification of a merging system. Overall the galaxy is relatively faint, and has a relatively small angular size on the sky.
