The galaxy presents as a single, largely featureless object. It appears elliptical in shape, exhibiting a high degree of central concentration and rotational symmetry. The color gradient transitions smoothly from a bright, yellowish core to a dimmer, reddish periphery. There is no discernible spiral structure or dust lane obscuration. The lack of distinct features suggests a relatively old stellar population, with limited ongoing star formation. The redder color at the edges may indicate the presence of older, cooler stars concentrated in the outer regions. A small fraction of tidal disturbances cannot be ruled out.
