The object presents as a spiral galaxy with a notable disk structure. The galaxy exhibits prominent spiral arms, tightly wound around a central bulge. The bulge appears relatively small compared to the overall disk size. The color distribution suggests ongoing star formation, with bluer regions concentrated along the spiral arms, indicative of younger, hotter stars. There is some evidence of a bar-like structure crossing the central bulge, though it appears relatively weak. The galaxy's morphology is slightly disturbed, potentially indicating minor gravitational interactions or recent merger activity. Overall, the galaxy appears as a relatively well-defined spiral, exhibiting moderate levels of star formation and a possibly barred morphology.