The galaxy exhibits a predominantly smooth morphology, appearing largely featureless in the image. Its shape approximates an ellipse, with a moderate elongation. Color gradients are apparent, with a more pronounced yellow/orange hue towards the central region, possibly indicating an older stellar population in the core, and bluer tints extending outwards. There is slight asymmetry in the distribution of light. No obvious spiral arms or a distinct disk structure are discernible. The galaxy is not exhibiting any signs of a major ongoing merger, though a possible minor disturbance cannot be ruled out.
