This galaxy appears to be a relatively smooth and featureless elliptical galaxy. It exhibits a centrally concentrated bright core, with a more diffuse halo extending outwards. The galaxy's light profile suggests it is primarily composed of older stellar populations. There is a potential merging event occurring as a close interaction, or perhaps even a full-fledged merger, with a companion galaxy with what appears to be active star forming regions. The main galaxy has a slight elongation, deviating from a perfect spherical shape, with a faint disk being a possibility, it is in an in-between form. Signs of any major disturbances within the primary galaxy are subtle. Overall, this galaxy seems to be a evolved system in a dense environment.
