The galaxy appears to be an interacting system, exhibiting morphological disturbances indicative of a merger in progress. There are two distinct components visible, with the larger having a more concentrated luminosity profile, exhibiting a smooth, elliptical-like morphology. Its color suggests an older stellar population dominating the light output. The second component is less concentrated and displays a bluer hue, suggesting ongoing or recent star formation activity. The apparent distorted shape of both components and the potential tidal features indicate gravitational interaction between the galaxies. There is an overall diffuse halo surrounding the system.
