The galaxy presents as a merging system, comprised of what appears to be at least two distinct, luminous components. Both components appear relatively smooth in morphology. The brighter, primary component exhibits a more circular shape, while the secondary component appears slightly elongated and shows evidence of tidal disruption or interaction. Faint tidal features or bridges seem to connect the two luminous regions, suggesting a gravitational interaction in progress. The overall color is reddish-yellow, indicating an older stellar population with relatively low ongoing star formation. There is some indication of minor dust lanes within the secondary component, evidenced by the slight color variations within its structure.
