The galaxy presents as an elliptical structure with a smooth, centrally concentrated light distribution. The morphology appears largely undisturbed, lacking prominent spiral arms or tidal features indicative of recent major mergers. The galaxy exhibits a subtle color gradient, transitioning from a somewhat bluer hue in its outer regions to a slightly redder core. This color gradient could suggest a population of younger, bluer stars in the galaxy's outskirts with older, redder stars congregated more centrally. Overall, the light distribution is quite smooth and the shape is highly circular.
