The galaxy presents a generally smooth, elliptical morphology. Its overall color appears yellowish-orange, indicating an older stellar population with fewer young, blue stars. A central bulge is visible, appearing brighter and more concentrated than the surrounding disk. The galaxy is elongated, suggesting a possible transition between elliptical and lenticular types. Faint hints of spiral structure may be present, though largely obscured by the dominant bulge. There is no strong evidence of active star formation regions or significant dust lanes. The galaxy appears relatively undisturbed, showing no strong signs of recent mergers or tidal interactions, though subtle features might be indicative of minor disturbances.
