The galaxy appears to exhibit a morphology suggestive of a system undergoing, or having undergone, a significant interaction or merger event. A primary, relatively smooth and centrally concentrated component is evident, displaying a slightly elongated, but generally rounded, shape. This central region appears brighter and possibly older, indicated by its reddish hue.

A secondary component, appearing bluer in color, is situated adjacent to the primary component. The bluer color may indicate a region of recent or ongoing star formation. This secondary component seems less defined and more diffuse than the primary component, potentially exhibiting tidal features or distortions indicative of gravitational interaction.

There is a suggestion of disturbed morphology. While a definitive tidal tail is not readily apparent, the irregularity in shape, particularly around the bluer component, implies a disturbance to the galaxy's structure. The overall light distribution is not uniform, hinting at a complex interplay of stellar populations and ongoing dynamical processes within the system.
