The galaxy presents a generally smooth and rounded morphology. The central region exhibits a bright, concentrated luminosity. The light distribution becomes more diffuse towards the outer edges of the galaxy, lacking any apparent spiral arm structure or distinct features. There is a slight elongation in the shape, but the overall structure remains predominantly elliptical. The color profile indicates a yellow-red hue, suggesting an older stellar population. The lack of blue light emission points to a lower rate of current star formation activity within the galaxy. There is no evidence of a major ongoing merger, although subtle disturbances in the outer regions are not ruled out. Overall, it presents as a fairly undisturbed elliptical galaxy.
