The galaxy presents as a somewhat diffuse object, exhibiting a disturbed morphology. A primary, brighter region shows a bluish hue, possibly indicative of recent or ongoing star formation activity. The light is not uniform but appears clumpy. The galaxy exhibits a faint extension or tidal tail, suggesting possible gravitational interactions or a past merger event. A secondary region, somewhat detached from the primary body, displays a more reddish color, potentially indicating an older stellar population or higher dust content. Overall, the galaxy does not appear to have a well-defined structure.
