The galaxy presents as a spiral type, viewed at an angle slightly off from face-on. Prominent spiral arms are visible, exhibiting a clumpy structure indicative of active star formation. These arms appear relatively open, with a noticeable blueness, likely due to the presence of young, hot stars. A central bulge can be discerned, although it appears relatively small compared to the overall disk size. The color of the bulge is yellower in comparison to the blue spiral arms, suggesting an older stellar population. A subtle bar feature seems to cross through the center of the galaxy. The disk itself is the dominant feature. No significant signs of tidal disturbances or ongoing major mergers are readily apparent. Overall, the galaxy appears to be a relatively undisturbed spiral system with a high degree of star formation activity.
