The galaxy exhibits an irregular morphology indicative of a system undergoing a major interaction or merger. The primary component appears relatively smooth in its central region, but possesses significant disturbances in its outer structures. Noticeable tidal features, potentially tidal tails or bridges, extend outward from the main galactic body, suggesting gravitational disruption. The color distribution is uneven, with a central concentration of yellowish-white light, possibly indicating an older stellar population. Regions of bluer light are also present and seem concentrated within the disturbed structures, which may indicate areas of active star formation triggered by the interaction. The galaxy displays an overall moderate size.
