The galaxy presents as a grand design spiral with two prominent, loosely wound arms emanating from a moderately sized central bulge. The arms display a patchy texture, indicative of active star formation regions interspersed with areas of lower density. These star-forming regions exhibit a bluer color, suggesting the presence of hot, young stars. Dust lanes are faintly visible along the inner edges of the spiral arms, contributing to the overall structure. The central bulge appears yellowish-white, possibly indicating an older stellar population. The disk is viewed at a relatively small inclination. There is no indication of a strong central bar. Subtle disturbances in the outer arms hint at potential minor gravitational interactions, but no major merger events are evident.
