The galaxy appears to be an elliptical galaxy with a smooth, symmetrical morphology. The light distribution is centrally concentrated, with the brightest region in the center gradually fading outwards. There is no obvious presence of spiral arms or a prominent disk structure. The galaxy exhibits a yellowish-red hue, suggesting an older stellar population with relatively low levels of ongoing star formation. The color gradient is subtle across the galaxy. There are no distinct features like tidal tails or obvious signs of recent merger activity observed, but some minor disturbances can't be ruled out at this resolution. The galaxy appears relatively undisturbed.
