The galaxy presents as an elliptical morphology, appearing relatively smooth and centrally concentrated. There is a slight elongation to the galaxy's shape. The core exhibits a bright, intense luminosity which gradually decreases towards the outer edges. The galaxy does not show any obvious spiral arm structures or strong dust lane features. The overall color appears slightly redder, suggesting an older stellar population. There is no apparent indication of any major ongoing merger events or significant tidal disturbances. The light profile appears consistent with a bulge-dominated system.
