The galaxy presents a spiral morphology, exhibiting a disk-like structure. The spiral arms are well-defined, emanating from a central bulge. The arms are moderately wound, with a primarily two-arm structure, and appear somewhat flocculent in nature. The bulge appears moderately sized and is characterized by a yellowish hue, indicative of an older stellar population. The disk shows evidence of active star formation, displaying a bluer color. Overall, the galaxy appears relatively undisturbed, without major signs of an ongoing merger, though minor tidal disturbances cannot be ruled out. The galaxy appears inclined at an angle which doesn't significantly obstruct the observer's view of the spiral arms. There may be a weak bar structure in the central region, although it is not clearly defined.