The galaxy presents as a relatively smooth, elliptical morphology. Its core is a bright, concentrated yellowish-orange hue, indicating an older stellar population. The intensity of this central region decreases gradually towards the outer edges, suggesting a radial decline in stellar density. The overall shape appears mostly spheroidal, but with a subtle elongation. There is no clear evidence of spiral arm structures or dust lanes, which further supports its classification as an elliptical galaxy. Faint, diffuse light extends from the central region, indicating a larger, less concentrated halo of stars surrounding the main body. No significant tidal features or signs of recent major mergers are readily apparent, though a slight asymmetry could indicate a minor past interaction.
