The galaxy presents as a disturbed system, potentially undergoing a significant merger event. A considerable amount of tidal debris is visible emanating from the primary body, indicating strong gravitational interactions. The main galactic structure exhibits a distorted morphology; any discernible spiral arms or a central bulge are obscured by the ongoing interaction. The primary body appears elongated, deviating significantly from a circular shape. Colors are indicative of intermediate-age stellar populations. The overall appearance suggests a system with an actively evolving morphology and enhanced star formation activity, possibly triggered by the ongoing merger. The galaxy is not particularly compact.
