The galaxy exhibits a centrally concentrated morphology with a bright, prominent core. There appears to be a diffuse, extended halo surrounding the core. The color profile suggests a relatively redder core with bluer arms or outer regions. The overall shape could be described as elliptical or possibly a spiral galaxy with tightly wound arms. There is evidence of a potential ongoing merger event or tidal interactions that appear to be significantly disturbing the structure. The symmetry is disrupted, and there are irregular features in the outer regions, suggesting gravitational interactions.
