This galaxy exhibits a disturbed morphology, suggestive of potential interactions or mergers. There is a main, elongated body with a bright central region. The light distribution is not uniform, and shows a clumpy appearance. Distinct asymmetry can be observed in the halo of the galaxy. There appears to be at least one secondary body close to the main galaxy, which is likely undergoing a minor merger with the main object. This secondary body is quite bright and compact. There are signs of tidal features or distorted structures. This is suggestive of on-going gravitational interaction between these two galaxies.
