The galaxy appears to be in a state of merging or undergoing a significant interaction. Two distinct, luminous components are visible, one displaying a reddish hue and the other a yellowish-white color. The reddish component is more compact and defined. The yellowish-white component is more diffuse and appears slightly elongated along the horizontal axis.

There is some morphological disturbance in the galaxy, suggesting gravitational interactions are ongoing. The overall shape is somewhat irregular, with no clear spiral arm structure discernible. There may be faint tidal features extending from the main body, but the image resolution limits clear observation of these.

Given the color differences, it is possible that the reddish component contains older stellar populations or a higher dust content, while the yellowish-white component may be actively forming stars. More spectral data would be needed to determine composition.
