The galaxy exhibits a somewhat amorphous structure, lacking a clear spiral arm definition or pronounced central bulge. Its overall shape appears flattened and disk-like. It shows signs of possible tidal disturbance or ongoing interactions, the asymmetry suggesting a recent or ongoing gravitational influence from an external source. I see what may be some tidal tails with lower surface brightnesses. The galaxy exhibits a bluer hue in some areas, suggestive of active star formation. Some redder regions could indicate a population of older stars or areas obscured by dust. There is some smoothness observed, but it is difficult to ignore the signs of a galactic merger occurring.
