The galaxy presents as a largely smooth, centrally concentrated object. Its overall shape is elliptical, appearing mostly round with a slight deviation towards a cigar shape. The light distribution within the galaxy shows a strong central bulge that emits significantly brighter light, fading in intensity towards the outer regions. There is minimal visible structure, such as spiral arms or dust lanes, suggesting a lack of significant ongoing star formation. Faint disturbances are observed, indicating a possible past interaction or minor merger event. The colors appear redder and slightly more dominant in the core region, and more blue in the outer layers, in accordance with its measured spectral properties.
