The galaxy appears as a relatively smooth, elliptical-like structure. The light distribution is concentrated towards the center, with a gradual decrease in intensity outwards. The galaxy's shape is generally rounded, with only a very slight elongation. There is no apparent spiral structure or distinct features suggestive of a disk component. The galaxy presents a subtle color gradient, transitioning from a somewhat bluer hue in its upper portion to a redder hue in its lower portion. No signs of major mergers or significant tidal disturbances are visually apparent. The overall appearance suggests an evolved stellar population with relatively low current star formation activity.
