The galaxy presents as a likely elliptical or lenticular type, appearing relatively smooth and lacking prominent spiral arm structures. It has a somewhat elongated, in-between roundness, not perfectly spherical but also not highly flattened.

The galaxy displays a dual-core structure suggesting a recent or ongoing merger event, the two nuclei are prominent and distinct.

The galaxy exhibits a yellowish hue, indicative of an older stellar population with diminished recent star formation. The overall light distribution appears centrally concentrated with a gradual decline in brightness towards the edges.
