The galaxy appears to be a relatively smooth, lenticular or early-type spiral galaxy, likely at a redshift of approximately 0.23. Its shape is noticeably elongated, appearing somewhere between round and cigar-shaped. There is a clear central bulge that is bright and concentrated, surrounded by a fainter, more diffuse disk. Within the disk, faint spiral arm structures may be present, though these are not distinctly defined. Color gradients suggest the presence of different stellar populations, with a redder core possibly indicating older stars and a more prominent population of younger stars in the disk. The galaxy doesn't show strong signs of any major ongoing merger events or significant tidal disturbances.
