The galaxy exhibits a generally smooth morphology, with a high degree of central concentration. The light is dominated by yellowish hues, suggestive of an older stellar population. There is evidence of a faint, slightly flattened, disk-like structure surrounding the central bulge. The overall shape is somewhere between round and elliptical, and there are no obvious signs of recent major mergers, although the outer regions show some subtle asymmetries that could potentially indicate minor disturbances. The color gradients indicate that star formation is likely low. The galaxy appears to be a relatively massive system.
