The galaxy presents as a somewhat elliptical structure, exhibiting a smooth, featureless morphology. The color gradient suggests a centrally concentrated population of older stars, appearing as a warmer hue that transitions to cooler, bluer tones in the outer regions.  The light distribution indicates a smooth spheroid, lacking any discernable spiral arms or bar structures. The axial ratio implies a moderate degree of ellipticity.  No apparent signs of recent or ongoing major mergers are observed, although there may be some minor asymmetrical features present, hinting at possible past interactions.  The overall appearance is consistent with a galaxy that has largely exhausted its gas supply, resulting in a lower star formation rate compared to actively star-forming galaxies.
