The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. Its overall shape is elongated, appearing as a flattened spheroid rather than a perfect circle. The light distribution is brightest in the core, fading gradually towards the edges, suggesting a centrally-dominated stellar population. The galaxy exhibits a slight color gradient, transitioning from bluer hues in the central region to slightly redder tones in the outer regions. This color change could indicate differing stellar populations or dust content. There may be evidence of minor disturbances in the galaxy's structure, specifically a slight asymmetry or possible tidal features, hinting at a past or ongoing gravitational interaction. No distinct spiral arms or a well-defined disk are apparent, supporting the classification as an elliptical galaxy. Based on the blue color in the core, there could be some star formation, but at a very low rate.
