The galaxy appears to be a relatively smooth, elliptical galaxy. The light profile suggests a high degree of central concentration, with a bright, yellowish core that fades gradually outwards. The overall shape is somewhat elongated, but not highly flattened, appearing roughly spheroidal. There is little evidence of spiral arms or distinct features within the galaxy. The light is dominated by redder wavelengths, indicative of an older stellar population. Faint blue light is also visible, suggesting a small amount of ongoing star formation. There is no apparent major interaction or merger occurring with another galaxy. Small signs of minor disturbance may be visible in the outer reaches of the galaxy.
