The galaxy appears to be part of a merging system. It presents with a primary component and a smaller, secondary component in close proximity.

The primary component exhibits a bright, compact core, surrounded by a more diffuse halo. There is evidence of tidal disruption or distortions in its overall shape, possibly due to gravitational interactions. The light distribution is not uniform, showing a complex structure. The galaxy's color suggests a mix of stellar populations, with bluer regions indicating younger stars.

The secondary component is smaller and also appears to be relatively compact. Its shape is somewhat irregular. There is also a blue color, potentially highlighting ongoing star formation.

Both components are embedded within a faint, extended envelope of light.
