This galaxy presents a disk-like morphology, oriented at a significant inclination relative to our line of sight. There is evidence of a central bulge. Subtle color variations across the disk suggest differential stellar populations or dust obscuration. A slight asymmetry in the light distribution hints at possible gravitational interaction or recent merger activity. The overall color profile appears moderately blue, indicating the presence of some younger stellar populations, but also shows redder regions, possibly indicating areas of older stars or dust presence. Further spectroscopic analysis is necessary to confirm the redshift, stellar populations, and star formation rates.
