This galaxy appears to be an elliptical, with a smooth, centrally concentrated light distribution. There is no apparent spiral structure or distinct disk. The galaxy exhibits a gradual decrease in surface brightness from the core outwards. The color is consistent with an older stellar population, with a yellowish-white central region that transitions to a slightly bluer hue in the outer regions, indicating a possible presence of younger stars in the outskirts, although limited. The galaxy's shape appears approximately round. There is no obvious evidence of major mergers or tidal disturbances in this image, although some minor asymmetry might be present.
