The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology is primarily elliptical in nature with a high degree of roundness. There is a minor disturbance visible, but its overall symmetry suggests that it has not undergone any major merging events recently. The color is a yellowish-white, which indicates a likely lack of significant ongoing star formation. The galaxy displays some extended light distribution, with a gradual decrease in brightness from its core outwards, suggesting an aging stellar population. The relatively red color implies a population of older stars that have shifted towards the red end of the spectrum.
