The galaxy presents as two distinct luminous components, with one appearing more spherical and yellow-white in color, and the other more spherical and reddish-orange in color. There is a potential interaction or overlap of these components. The brighter yellow-white component shows a smooth, indistinct morphology, whereas the dimmer reddish-orange component has slightly less uniform color distribution. Neither component exhibits distinct spiral arms or a well-defined galactic disk. The galaxy displays an overall disturbed morphology, potentially indicating an ongoing or recent merger event. Based on color, the overall star formation appears to be suppressed.
