The galaxy presents as a merging system comprised of at least two distinct components. The larger of the two exhibits a predominantly smooth morphology, with a high degree of central concentration and a relatively round appearance. Its color is generally yellow, indicative of an older stellar population. The second, smaller component is positioned in close proximity, potentially interacting tidally with the larger galaxy. It also appears relatively smooth. A faint tidal tail is visible, suggestive of gravitational interaction. This merging system displays a low level of recent star formation activity. The system exhibits significant luminosity, suggesting a relatively high stellar mass.
