The galaxy presents as a likely merging system, characterized by significant morphological disturbance. There are two primary components to the system, each with distinct properties.

The first component appears bluer in color, with a slightly elongated morphology. There is an indication of possible tidal features emanating from this component, contributing to the overall disturbed appearance.

The second component exhibits a more yellowish-red hue, suggesting an older stellar population. This component also shows signs of interaction, with the morphology seemingly disrupted.

The overall system displays a complex structure indicative of ongoing gravitational interaction. The presence of tidal features and the disrupted morphologies of both components support the assessment of an active merger event. The system's light distribution is uneven, suggesting recent or ongoing star formation activity.
