The galaxy presents as a spiral with a noticeable disk structure. The central bulge appears relatively small and unobtrusive, gradually transitioning into the disk. The spiral arms are well-defined and exhibit a flocculent morphology, displaying a patchy distribution of star-forming regions. The arms are primarily composed of two main arms, extending from the central region. There may be traces of a bar-like structure within the central region, though it does not appear exceptionally strong. The overall color profile suggests ongoing star formation, with hints of blue indicating populations of young, hot stars within the spiral arms. There might be a minor gravitational disturbance in the disk of the galaxy. 
