The galaxy appears to be an elliptical galaxy, exhibiting a smooth, symmetrical morphology with a centrally concentrated bright nucleus. The color gradient indicates a population of older stars. It presents a generally round shape, showing little evidence of a disk-like structure or significant tidal disturbances. Based on the observed light distribution, star formation activity seems low, the overall color suggesting it may be a quiescent galaxy. There are no apparent signs of ongoing mergers or interactions with other galaxies.
