The galaxy appears as a centrally concentrated object with a smooth light distribution, suggesting an elliptical morphology. The galaxy is elongated, with a moderate axial ratio, indicating a slight flattening. A lack of distinct spiral arm structures or prominent dust lanes suggests an older stellar population dominating the galaxy's composition. The light is relatively uniform and the color appears to be generally blue-white, possibly indicating a mix of stellar populations and some active star formation. There might be minor disturbances or interactions present, but the overall structure appears relatively undisturbed.
