The galaxy presents a complex morphology, suggestive of an ongoing or recent interaction or merger. The central region exhibits a bright, compact core with a distinct bluish hue, possibly indicative of active star formation within a concentrated area. A notable extension or arm emerges from the core, displaying a more yellowish color. This could signify an older stellar population, dust, or a different composition compared to the core. The overall structure lacks a clear spiral or elliptical form, indicating a disturbed morphology, possibly caused by tidal forces. Faint wisps or diffuse light are observed extending outwards from the main body of the galaxy, which could be stellar material ejected during the merger.
