The galaxy appears to be a somewhat elongated elliptical galaxy at a redshift of approximately 0.23, indicating substantial distance. The galaxy’s central region exhibits a bright, concentrated luminosity, with a yellow-white hue, suggesting a high concentration of older stellar populations. The outer regions show a gradual decrease in surface brightness, fading into a more diffuse halo. The overall color is consistent with an aging stellar population, with a slightly redder tint in some regions possibly indicating the presence of dust or a small amount of ongoing star formation. There is very slight evidence of tidal disturbances on either side of the galaxy. It seems to be relatively isolated, not showing strong signs of interaction with other nearby galaxies. The galaxy’s light distribution is smooth, with little visible structure, giving it an elliptical morphology.
