The galaxy presents as a single, dominant spheroidal structure with a smooth appearance, indicating an elliptical morphology. It exhibits a concentrated central bulge that appears nearly circular. There is a lack of any discernible spiral arms, bar structures, or strong dust lanes. Color gradients suggest that the galactic core is likely composed of older stellar populations. The overall yellow-red hue may indicate that this is a relatively evolved galaxy with low rates of current star formation. There appears to be no signs of any recent or ongoing merger events or major tidal disturbances. The outer regions fade gradually, indicating a smooth transition to the intergalactic medium.
