The galaxy presents as a somewhat irregular, disk-like structure. Its morphology is dominated by a central, bright region exhibiting a diffuse, bluish hue, suggesting ongoing or recent star formation. The overall light distribution is uneven, hinting at internal disturbances or interactions. A faint, extended tail or plume extends outward from one side of the main body, potentially indicating tidal stripping or a past merger event. There isn't a clearly defined spiral arm structure visible in this image. The central bulge is not prominent, possibly even absent or obscured by the brighter star-forming regions. Evidence of merging is present due to disturbances in the shape.
