The observed galaxy exhibits a distinct spiral morphology. Two prominent spiral arms emerge from a central bulge. These arms appear to be moderately wound. There are no signs of major interaction or merging events. The color of the galaxy suggests ongoing star formation activity, particularly in the spiral arms. The bulge appears more yellow, potentially indicating an older stellar population compared to the bluer arms. The disk is oriented face-on, allowing for a clear view of its spiral structure. There may be a weak bar structure present at the galaxy's center, but it is not distinctly visible. The central bulge appears moderate in size relative to the overall disk.
