The galaxy presents as a grand design spiral with prominent, well-defined spiral arms. A central bulge is apparent, though not highly pronounced. The spiral arms exhibit a flocculent structure, appearing somewhat patchy with varying densities of stellar populations and gas. These arms display a moderately open winding. The color gradient across the galaxy suggests ongoing star formation, particularly within the spiral arms where blue hues indicate the presence of young, hot stars. The galaxy's disk appears relatively thin. Evidence of a possible bar structure cutting through the center of the galaxy can be seen, causing some asymmetry in the inner regions. There is also evidence of possible interactions or disturbances, as suggested by slight distortions in the outer spiral arms.
