The galaxy presents as a relatively smooth, elliptical-like structure. Its light profile indicates a concentrated central bulge that decreases in intensity radially outward. There is a subtle color gradient observed, with the core appearing slightly yellower than the outer regions, which tend towards redder hues. This suggests an older stellar population dominating the central region, with potentially younger, hotter stars located in the outer parts of the galaxy. No distinct spiral arms or significant dust lanes are immediately apparent. There may be slight disturbances in its overall form, suggesting a potential minor interaction event, but it has a generally round shape. Overall, the galaxy exhibits characteristics consistent with a evolved system exhibiting low rates of star formation.
