This galaxy exhibits a complex morphology indicative of ongoing or recent interaction. The central region appears diffuse and somewhat elongated, showing a yellow-green hue that may indicate a moderate amount of star formation. A plume-like extension emanates from this central area, displaying a bluer color suggestive of a younger stellar population.

The overall structure shows signs of disturbance.  Arms are not clearly defined and the general shape is irregular. Patches of bluer light scattered within the galaxy further suggest localized star-forming regions. There appears to be a faint redder component enveloping the central structure, which could represent an older stellar population. The lack of a well-defined nucleus and the disturbed morphology suggest the possibility of a recent or ongoing merger event.  Distinct tidal features, such as extended streams of stars, are not obviously visible, but low surface brightness features may be present in deeper imaging.
