The galaxy presents as a somewhat distorted disk galaxy, with an approximate effective radius of 1.2 arcseconds. The central region of the galaxy exhibits a bright core, with a slightly elongated structure. There is a hint of spiral arm structure, but it appears disrupted, especially on the upper left side of the image. The color distribution indicates varying stellar populations and dust content within the galaxy. The inner regions show a bluer coloration, perhaps indicating younger stars, while the outer regions show a shift to redder colors. The overall morphology suggests a possible recent or ongoing interaction or merger event, indicated by the disturbed arms.
