The galaxy presents as a relatively smooth, elliptical-like structure. Its central region exhibits a concentrated luminosity, transitioning outward to a less intensely illuminated halo. The galaxy's shape appears predominantly rounded with a slight elongation. There is no clear evidence of major mergers or significant tidal disturbances in the immediate vicinity. A subtle color gradient is observable, with the core trending towards yellower hues, possibly indicating an older stellar population compared to the outer regions where hints of redder tones can be seen. The overall structure suggests a system in a fairly relaxed state, lacking the pronounced features often associated with active star formation or recent merger events.
