The galaxy presents as an elliptical morphology, with a smooth, diffuse light profile. The core region exhibits a higher concentration of luminosity, appearing a more intense yellow, suggesting an older stellar population. The outer regions fade gradually into the background, with a more diffuse, slightly bluer hue, implying the presence of some younger stars, possibly from a low level of on-going star formation. The overall structure does not appear to be significantly disturbed, showing no signs of major mergers or tidal interactions, although there may be some minor irregularities in the outer regions. The galaxy's elongated shape suggests it is not perfectly spherical, but rather closer to an oblate spheroid. Overall, this galaxy appears to be a relatively massive, evolved system with a moderate redshift.
