The galaxy presents as a disturbed system. It appears to be undergoing a merger, or a period of significant gravitational interaction with another galaxy, as indicated by the asymmetrical morphology and extended tidal features. A clear disk component is not readily apparent, making classification as a spiral challenging without further data. There are noticeable regions of intense star formation within the galactic structure, evidenced by the localized concentrations of bluish-white light, suggestive of hot, young stars. Conversely, the presence of reddish-yellow hues implies the existence of older stellar populations or regions of dust obscuration. The overall luminosity suggests a massive system. The irregular shape and the tidal features indicate a dynamic and ongoing evolutionary process.
