The galaxy presents as a relatively smooth, centralized luminous object, roughly circular in appearance. There is a slight elongation present. The color profile is predominantly blue-white, suggesting the presence of a significant population of hot, young stars, which is characteristic of ongoing, or recent, star formation within the galaxy. The galaxy is compact, exhibiting a concentration of light toward its center. There is no discernible disk structure or spiral arm morphology visible in this imaging, with a smooth appearance, although there appears to be a slight disturbance on one side of the galaxy. No signs of a major merger is observed, and little dust is present. 
