The galaxy appears as a singular, concentrated body of light. It presents an elliptical morphology, exhibiting a smooth, featureless profile with a high degree of central concentration. There is no visible spiral arm structure or evidence of a prominent disk. The galaxy's color index suggests a dominant stellar population of older, redder stars, indicative of a quiescent or passively evolving system. There is a noticeable lack of blue light associated with active star formation regions. The object demonstrates a round shape and does not seem to be undergoing any major merging events or tidal disruptions based on the image.
