The galaxy presents as a dual-cored system, possibly indicative of an ongoing or recent merger. The two primary components exhibit a relatively smooth morphology, with a centrally concentrated luminosity profile in each core. One core appears slightly more elongated than the other. There is a subtle color gradient across the galaxy, with the brighter, more diffuse core exhibiting a slightly bluer hue compared to the slightly redder hue of the lower core. The overall structure appears relatively undisturbed despite the potential merger, with little evidence of tidal tails or strong distortions. The dominant fraction of the light comes from a smooth component, indicating this system is dominated by older stellar populations with some evidence of recent star formation.
