The galaxy presents a somewhat inclined disk morphology. Two prominent spiral arms are discernible, exhibiting a loosely wound structure extending outward from the central region. The arms display a mottled texture, suggesting areas of active star formation or dust obscuration. The central bulge appears moderately sized and exhibits a smooth, concentrated luminosity profile. The overall color of the galaxy is somewhat blue-green, indicating a population of relatively young, hot stars within the disk. There does not appear to be evidence of any major mergers, but there may be some minor disturbances.