The galaxy appears to be an interacting system, potentially in the early stages of a merger. One component displays a disk-like morphology, with a relatively smooth profile. The disk exhibits a notable tilt relative to our line of sight. There is some asymmetry in the light distribution of the disk, possibly indicative of tidal disturbances or ongoing star formation regions. The color of the disk exhibits bluer hues, which suggests the presence of younger stellar populations.

The second component appears more spheroidal in shape and is of a yellower hue, suggesting an older stellar population and potentially higher dust content. The overall structure is relatively concentrated, with a smooth luminosity gradient.

The system as a whole is elongated, with the two components appearing gravitationally bound and influencing each other's morphology. The separation between the two components is significant, but they are connected, possibly through a tidal bridge.
