The galaxy appears to be a relatively smooth, elliptical-like structure, exhibiting a concentrated central bulge. It possesses a generally rounded morphology, with no discernible spiral arms or significant asymmetries. The light distribution suggests a fairly even stellar population, with a gradient from a brighter, more yellowish core to a slightly fainter, more reddish outer halo. There is no apparent evidence of ongoing major merger activity or significant tidal disturbances, although minor perturbations cannot be ruled out. The overall color profile indicates a population dominated by older stars, with potentially suppressed star formation.
