The galaxy presents a prominent disk structure, viewed at an angle of approximately 30 degrees relative to edge-on.  Spiral arms are clearly delineated, exhibiting a tightly wound morphology.  There appears to be a relatively small but noticeable bulge component in the galactic center.  The arms show a bluish hue.  The arms are of intermediate prominence, some arms seem hard to distinguish from one another and somewhat intertwined. No major signs of mergers are clearly observed, though there is some structural irregularity hinting at potential minor gravitational interaction. Star formation appears to be moderately active within the spiral arms as indicated by a population of blue stars. The galactic disk is well defined and prominent.  The central bulge shows yellow to red colors.  The galaxy displays a relatively symmetrical appearance with a somewhat disturbed overall structure.
