The galaxy appears to be a spiral type, presented at a near face-on orientation. Two prominent spiral arms are clearly visible, exhibiting a loose winding pattern. The arms display a patchy, somewhat flocculent structure. The central bulge appears relatively small and indistinct; the galaxy is dominated by its disk. A bar structure can be inferred running through the core of the galaxy. No major signs of merging are observed, although there may be some minor disturbances. The color suggests a actively star-forming galaxy, with a blue hue noticeable in the spiral arms.
