The galaxy presents as a single, relatively smooth concentration of light, appearing elliptical in shape. The object exhibits a core region of high luminosity, with a yellow-orange hue, indicating an older stellar population. The light gradually diffuses outward from the core, lacking any distinct spiral arm structures or other prominent features. The absence of defined structures suggests a lack of significant ongoing star formation. The overall appearance points towards an evolved galaxy with a substantial spheroidal component. There is a subtle deviation from perfect sphericity; however, the galaxy appears generally relaxed and undisturbed.
