The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. It exhibits a significant spheroidal component, appearing largely featureless without obvious spiral arm structures or dust lanes. The color profile indicates an older stellar population, with the core region displaying a yellow-orange hue, suggesting a dominance of evolved stars. There is a gradual color gradient extending outwards, where the outer regions display a slightly redder tint. The overall roundness of the galaxy is indicative of an E type galaxy. The relative uniformity of the color profile and the lack of significant irregularities suggest that the galaxy is not undergoing any major mergers or significant starburst activity, however there may be low-level star formation occurring. The galaxy appears generally undisturbed with no apparent tidal tails or distortions.
