The galaxy presents as a relatively compact, luminous object. Its morphology appears largely smooth and elliptical, with a high degree of circularity. There are no discernable spiral arms or a bar structure visible. Faint traces of minor disturbances may be present, but these are difficult to confirm conclusively. The light profile suggests a concentration of older stars and it is likely a highly massive system, with an apparent size of ~9 kpc. The color index, estimated from the limited spectral information available, is approximately red, suggesting a population of relatively old stars. The galaxy does not show obvious signs of ongoing major star formation.
