The galaxy presents as an elliptical morphology, appearing largely smooth and centrally concentrated. Its color profile indicates an older stellar population, with a pronounced red-yellow hue concentrated towards the nucleus. There is little evidence of spiral arms or significant dust lanes, and a lack of prominent blue regions suggestive of active star formation. The galaxy exhibits a degree of roundness, deviating only slightly from a perfect sphere. There is no evidence of ongoing or recent major mergers or tidal disturbances. The galaxy appears to be isolated and relatively undisturbed within its immediate environment.
