The galaxy presents a morphology consistent with an elliptical type. It appears largely smooth and featureless, lacking prominent spiral arms or a well-defined disk structure. The galaxy exhibits a centrally concentrated light profile, with the luminosity decreasing gradually outward. The overall shape is close to round. There is a hint of some tidal disturbances, possible signs of a past merger. The galaxy is on the bluer side, suggesting ongoing star formation, though that star formation may not be very intense.