This galaxy appears to be largely smooth and elliptical in shape. There is a noticeable lack of defined spiral arms or a prominent disk structure. The light distribution is fairly uniform, with a gradual fading towards the edges. The color profile suggests a redder overall hue, possibly indicating an older stellar population. There appears to be some degree of disturbance in the morphology, potentially due to a minor interaction. The overall structure leans towards a rounded shape. Based on these observations, this could be classified as an elliptical galaxy experiencing some tidal disruption.
