The galaxy presents as a binary system undergoing tidal interaction. One component appears as a centrally concentrated spheroid, exhibiting a smooth light profile. The core displays a bright, likely active galactic nucleus, surrounded by a fainter, diffuse halo. A tidal bridge links this spheroidal component to a second, less well-defined component that appears more diffuse and elongated, consistent with significant tidal disruption. Evidence of recent or ongoing star formation within the spheroidal core is suggested by its slightly blue-shifted color relative to the overall system. The distorted morphology of the second component is indicative of a significant gravitational interaction. The overall system exhibits a notable luminosity suggesting a relatively high stellar mass.
