The galaxy appears to be undergoing a significant interaction, possibly a merger, with another galaxy. The primary galaxy exhibits a relatively smooth, concentrated core suggesting an older stellar population. Diffuse light extends from the core, indicating a spheroidal component with a size of approximately 6 kpc in radius.

A secondary object is observed in close proximity. This companion displays disturbed morphology and a brighter area with a bluish color, hinting at younger star formation. Tidal features, potentially faint tidal tails or bridges, appear to connect the primary galaxy with the secondary object, indicating a gravitational interaction. The degree of disturbance suggests a major interaction is underway or has recently occurred.
