The galaxy appears to be undergoing a merger. The primary component of the galaxy exhibits a relatively smooth morphology, with a somewhat elliptical shape. There's a suggestion of a central bulge and a faint disk, though resolution is limited. The light distribution is fairly concentrated. A secondary object, possibly a smaller galaxy or tidal debris, is interacting with the primary galaxy. This object shows a more irregular morphology, with a redder color, potentially indicating older stellar populations or dust obscuration. The overall color of the system suggests a mix of stellar ages, with some regions exhibiting bluer colors indicative of ongoing star formation. Evidence of minor disturbance in the main body can be seen, which might also indicate there is a possible interaction with a third object that cannot be resolved.
