The galaxy presents a predominantly smooth morphology, with minimal discernible features suggesting a disk-like structure. Its overall shape appears to be roughly rounded, exhibiting a slight deviation from perfect circularity. The galaxy's light profile suggests a concentrated central bulge with a gradual decrease in intensity towards its outer regions. Color gradients indicate a higher concentration of older stellar populations within the core, characterized by yellowish hues, while bluer tones in the outer regions might suggest the presence of some younger stars or ongoing, but weak, star formation. There's no strong evidence of active merging or significant tidal disturbances, although subtle asymmetries could indicate minor past interactions. Based on its red color and smooth structure, this galaxy appears to be a massive elliptical galaxy.
