The galaxy presents as a pair of distinct structures, possibly interacting or in close proximity. One structure exhibits a bluer hue, suggesting the presence of younger stellar populations and potentially ongoing star formation. This component displays a somewhat diffuse appearance. 

The other is characterized by a yellower color, indicative of older stellar populations. Its light is more concentrated in the galaxy's center. The overall morphology of the system appears to be elliptical, with a smooth, rounded shape. There are no clear signs of spiral arms or a prominent disk.

The structures exhibit some distortion, indicating potential gravitational interaction. There may be faint tidal features.
