The galaxy presents as a spiral type, observed at a moderate redshift. The disk is viewed at an angle slightly off from face-on, exhibiting a notable degree of disruption in its structure. Evidence of spiral arms is present, though these are not sharply defined. The galaxy shows signs of tidal disturbances, possibly indicating an ongoing or recent interaction with another galaxy or minor merger event. The bulge appears moderate in size, with the disk's luminosity being a notable feature. The central region exhibits a concentrated yellowish hue, transitioning to bluer shades in the outer arms, indicative of a mix of older stellar populations in the core and younger stars in the spiral arms. There is a distinct color variation present, with localized regions possibly experiencing active star formation. Overall, the galaxy appears to be a dynamically active spiral with a history of interaction.
