This galaxy appears to be a disk galaxy seen at an oblique angle, not quite edge-on but tilted significantly from face-on. The central bulge region is prominent, exhibiting a smooth, yellowish-white glow, suggesting an older stellar population dominates this area. Surrounding the bulge, there is evidence of a flattened disk structure. Within the disk, there are hints of spiral arm structures, indicated by patches of bluer light, which likely signify regions of ongoing star formation. The disk also shows greenish hues, potentially indicating the presence of ionized gas. There is an apparent tidal tail or a merging dwarf galaxy visible on one side of the main galaxy. It looks like a separate smaller redder and compact object next to the galaxy, suggesting recent or ongoing interaction. Overall, the galaxy has a disturbed morphology, possibly due to the interaction.
