The galaxy presents as an interacting system. A larger, somewhat amorphous component dominates the scene. It is centrally concentrated with a diffuse, extended halo exhibiting a subtle blue tint, suggestive of ongoing, albeit potentially low-level, star formation. The overall morphology is neither distinctly elliptical nor spiral.

A second, smaller component appears as a flattened disk, oriented edge-on relative to our line of sight. This disk exhibits a more pronounced blue color, indicating more active star formation relative to the larger component. This secondary galaxy displays a smooth structure, with no obvious spiral arm features visible.

The proximity and distorted appearance of both components imply a gravitational interaction. This could manifest as tidal features or other distortions not clearly resolved in this image. There is evidence of merging activity.
