This galaxy exhibits a morphology suggesting a potential interaction or merging event. The central region appears somewhat amorphous, lacking a well-defined nucleus. A diffuse, elongated structure extends outwards, displaying a faint, tail-like feature on one side, which could be indicative of tidal forces. The overall color of the galaxy appears slightly redder, suggesting a population of older stars. There may be a small amount of active star formation, although subtle, there seems to be some bluer knots of light.
