The galaxy presents as a singular, relatively smooth, and concentrated distribution of light. Its overall morphology appears elliptical, with the luminosity profile gradually decreasing from the center outwards. The core region displays a bright, concentrated yellowish-white hue, suggesting a population of older stars. The surrounding halo exhibits a fainter, more diffuse light, fading into the background sky, and there are only the slightest hints of subtle color variations within the galaxy's structure, with the outer edges perhaps exhibiting a slightly redder tone. No distinct spiral arms or other prominent features are apparent, indicating a lack of significant ongoing star formation. There is no evidence of tidal disturbances or interactions with other galaxies. The overall impression is that of a relaxed, quiescent system.
