The galaxy presents an elliptical morphology, appearing somewhat flattened rather than perfectly spherical. The light distribution suggests a centrally concentrated bulge, with a gradual decrease in surface brightness toward the outer regions of the galaxy. The core exhibits a yellowish hue, potentially indicating an older stellar population. There may be some slight disturbances in the overall structure but it is hard to be certain. The galaxy has an apparent magnitude in the range of 16-18.
