The galaxy presents as an elliptical or lenticular galaxy with a smooth, centrally concentrated light distribution. There is no discernible spiral arm structure or distinct disk component visible in this image. The galaxy appears to be generally round in shape, with little to no elongation or distortion. The color profile reveals a yellow-orange hue in the core that subtly transitions to redder tones in the outer regions, suggesting an older stellar population with ongoing or recently ceased star formation. The absence of strong blue colors indicates a lack of significant ongoing, massive star formation within the observed timeframe. The galaxy appears isolated, with no obvious signs of tidal interactions or major mergers.
