The galaxy appears as a moderately luminous object with an elliptical morphology. It displays a smooth, generally featureless structure, showing little evidence of spiral arms or prominent dust lanes. The light distribution suggests a centrally concentrated stellar population, with a gradual decrease in surface brightness toward the outer regions. There is a slight elongation in shape, though it is mostly rounded. Evident distortions or signs of major mergers are not clear, but subtle disturbances or minor interactions cannot be ruled out. The color profile indicates the presence of evolved stellar populations.
