The galaxy presents as a complex system, exhibiting evidence of multiple interacting components. A prominent feature is a relatively bright, disk-shaped structure oriented nearly edge-on. This component displays a concentrated central bulge, appearing predominantly smooth and rounded. There is faint suggestion of dust-lane obscuration, with slightly darker regions bisecting the disk.

The main galaxy appears to be gravitationally interacting with one or more nearby objects, as indicated by tidal distortion. At least one less luminous object is present, with a less defined structure. The overall color of the system is trending towards a redder hue, suggesting an older stellar population and diminished current star formation, despite the evidence for interaction. The system appears to be undergoing a merger, possibly in the early stages. There is evidence of some disturbance, but no major disruption.
