The object presents as a galaxy with a complex morphology, likely undergoing an interaction or merger. There appears to be a primary, relatively smooth component, exhibiting a flattened shape, elongated along a northeast-southwest axis. This component has a yellowish hue, suggesting an older stellar population and/or significant dust obscuration.

Superimposed on the primary component are two distinct, bright, bluish knots. These features indicate regions of intense star formation. They appear relatively compact and possibly represent tidal dwarf galaxies or star-forming regions triggered by the interaction.

The overall structure is disturbed, showing signs of gravitational interaction. There may be faint tidal features extending from the main body.

The light profile exhibits no clear spiral structure, hinting towards an elliptical or irregular classification, heavily influenced by the ongoing merger. The galaxy appears to be of intermediate size, with no obviously dominant nucleus.
