The galaxy presents as a relatively compact, elliptical structure, exhibiting a smooth, diffuse light profile with no discernible spiral arms or bar. The galaxy is generally round in shape. There is a slight variation in the colour across the galaxy, with the central region appearing slightly more yellow/orange than the periphery, indicating a possible concentration of older stellar populations in the core, however the galaxy as a whole is orange leaning, suggesting an older galaxy that has ceased the majority of star formation. There is no evidence of active galactic nuclei activity or significant dust lanes. The galaxy does not appear to be undergoing any major mergers. The galaxy shows no apparent evidence of disturbance to its form.
