This galaxy exhibits a disturbed morphology, suggestive of an ongoing or recent merger event. A bright, yellowish central bulge is prominent. Emanating from this central region is a faint, blueish tail-like extension, possibly a tidal feature resulting from gravitational interaction. The overall structure is irregular and lacks a well-defined spiral arm pattern, further indicating a non-quiescent state. The colour gradient from the bulge to the tail suggests a difference in stellar populations, with the bulge likely containing older, redder stars and the tail potentially hosting younger, bluer stars formed during the merger process. Dust lanes or patches appear indistinct, possibly obscured by the tidal features.
