The galaxy presents as a largely featureless elliptical structure with a smooth luminosity profile. The color index suggests a higher concentration of older stellar populations, lending it an overall yellow-orange hue. There's no strong evidence of spiral arms or significant dust lanes. The galaxy's round morphology and undisturbed structure imply a relaxed dynamical state, with no signs of recent major mergers or interactions. The light distribution is centrally concentrated with a gradual fall-off towards the outer regions, with no sharp boundaries or breaks in the light profile detectable at this resolution.
