The galaxy presents as a centrally concentrated object with a smooth, largely featureless morphology. The light profile appears to be dominated by a centrally located bulge component that contributes most of the luminosity. The galaxy's shape is approximately circular. The light distribution exhibits a radial gradient, with the core being significantly brighter and yellower than the outer regions, which appear fainter and slightly bluer. There is little evidence of spiral arms or other disk-like structures. The color suggests an older stellar population. There is no obvious indication of active star formation. No tidal tails or signs of recent mergers are visible. The galaxy appears to be relatively isolated and undisturbed.
