The galaxy presents as an elliptical type, exhibiting a largely smooth and featureless morphology. Its shape is generally round, with a slight departure toward a more intermediate form. The core is comparatively bright, possibly indicative of a concentrated stellar population. There is a decrease in luminosity that seems to spread outwards. The galaxy does not show a strong presence of spiral arms or a well-defined disk structure. There are no visible signs of on going merger activity or major tidal disturbances.
