The galaxy presents as a disk galaxy with a prominent central bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population. The disk component of the galaxy shows evidence of spiral arm structure, though the arms are somewhat loosely wound and not sharply defined. There is some patchiness observed throughout the arms.

The galaxy's disk appears relatively face-on, and the arms emanate from the central bulge. The disk exhibits a bluer color profile, indicating the presence of younger, hotter stars and regions of active star formation within the spiral arms. 

A small companion object is visible near the galaxy. Whether this companion is gravitationally bound or a line-of-sight effect will require further study.

Overall, the galaxy appears to be a spiral galaxy of intermediate size, with ongoing star formation primarily concentrated within the spiral arms. There is no obvious active galactic nuclei.
