The observed galaxy presents a spiral structure, with a prominent central bulge. Spiral arms are visible, exhibiting a relatively flocculent morphology. The disk of the galaxy appears face-on, allowing for a clear view of its spiral features. The galaxy exhibits a slight blue tint, particularly concentrated in the spiral arms, suggestive of ongoing star formation. There is a subtle central bar feature. No significant signs of major mergers or strong tidal disturbances are apparent, though some minor asymmetry hints at possible past interactions. The bulge appears to be relatively small compared to the overall size of the disk. Overall, this galaxy seems to be a typical spiral with ongoing star formation and moderate structural features.
