The galaxy presents a smooth, elliptical morphology, lacking discernible spiral arms or a prominent disk structure. The light profile appears relatively concentrated toward the center, exhibiting a gradual decrease in intensity outwards. Its color is dominated by yellow and red hues, suggesting an older stellar population with a lower rate of ongoing star formation. There are no apparent signs of recent or ongoing major mergers or tidal disturbances. The overall appearance suggests a well-evolved system approaching a state of quiescence.
