The galaxy presents as a system with a primary, larger component and a smaller, distinct secondary component in close proximity. The primary component exhibits a generally smooth morphology, with a somewhat elliptical appearance. There is a subtle suggestion of internal structure, but it is not highly defined. Its color appears to be predominantly redder, indicating a stellar population that is potentially older and less actively forming stars.

The secondary component is smaller and rounder in appearance. Like the primary component, it also possesses a redder color, indicative of an older stellar population. There is the suggestion of a tidal tail or bridge connecting the two components, indicating a possible gravitational interaction or ongoing merger event. However, the image resolution limits a definitive determination. Overall, the system appears to be in an intermediate stage of interaction.
