The galaxy appears to be an elongated object, with a notably brighter central region, suggesting a concentration of stars and possibly a central bulge. The galaxy exhibits a disturbed morphology, which could be indicative of a galaxy merger. The light distribution is not uniform. The overall color appears somewhat blue, potentially implying the presence of younger stellar populations and ongoing star formation. There seems to be an irregular tidal tail extending away from the main body, indicative of gravitational interactions. The main body is relatively compact, yet diffuse and not clearly resolved. 
