The galaxy appears to be in a stage of interaction, exhibiting a dual-core morphology suggesting an ongoing or recent merger event. It is not clear if the two cores are of equal mass, but the lower core appears to be brighter and larger, giving the galaxy an elliptical form. The galaxy exhibits a generally smooth light profile, with no distinct spiral arms or prominent dust lanes visible, consistent with an early-type morphology or a late-stage merger remnant.

The overall color is yellowish-white, indicating an older stellar population, although bluer colors are evident as the galaxy fades into its edges.
