The galaxy appears to be part of a small group or interacting system. One component presents as a relatively smooth, elliptical galaxy with a concentrated, bright core, suggesting an older stellar population. A second component exhibits a bluer hue and slightly irregular morphology, indicative of ongoing star formation. This second component may be a disk galaxy undergoing tidal disruption or a dwarf galaxy interacting with the larger elliptical. There is a faint, diffuse bridge of light connecting the two main components. Finally, there may be a third smaller component to the system, suggesting that this galaxy is undergoing a merger. The overall appearance is that of a system in the midst of dynamical interaction.
