The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The color gradient transitions smoothly from a bright, yellowish core to a more diffuse, reddish halo. There is little to no evidence of spiral arms or significant dust lanes. The overall morphology suggests an evolved system, likely composed of an older stellar population. It appears generally round, with no obvious signs of major tidal disturbances or ongoing mergers. Minor irregularities may be present in the outer regions, but the resolution limits definitive assessment.
