This galaxy exhibits characteristics suggesting an ongoing or recent merger event. Two distinct luminous components are visible. One component appears as a more diffuse, elliptical shape, possibly indicative of a spheroidal galaxy or the bulge of a spiral galaxy. The second component shows a more defined, disk-like structure oriented at an angle. This could be another spiral galaxy interacting with the first. 

There is a faint tidal tail or bridge-like feature extending between the two main components and an additional tail like feature extending off of the second component. These are likely formed due to the gravitational interaction.

The overall color of the galaxy system appears yellowish, suggestive of an older stellar population, although there might be some obscured regions of more recent star formation, particularly in the more defined disk. The system shows signs of disturbances, and there may be a region of intense activity.
