The galaxy appears to be a spiral galaxy, observed nearly edge-on. A prominent disk structure is visible, exhibiting a relatively smooth light distribution. There is a central bulge that dominates the central region, appearing slightly flattened. The blue color suggests the presence of a population of young, hot stars and ongoing star formation, especially around the central area. Some light reddening seems to occur through the midplane of the disk, likely due to dust obscuration. No significant tidal disturbances or merging features are clearly discernible, suggesting it is a relatively isolated and undisturbed system. The galaxy appears to be well-defined with no major irregularities.
