The galaxy presents as an irregular, disrupted structure. A bright, concentrated central region is visible, exhibiting a bluish hue, which may indicate ongoing or recent star formation. Emanating from this central region is an extended, fainter component that curves around the central area. This feature is less defined, with a more diffuse appearance. The galaxy’s overall shape suggests a possible interaction or merging event. The extended component may represent tidal debris resulting from such an event. There are hints of reddish regions embedded in the central area. These could represent older stellar populations, regions of dust obscuration, or a combination of both. The galaxy shows indications of significant star formation activity.
