The galaxy appears to be an interacting system, comprised of two distinct galactic bodies. The primary galaxy presents a smooth, elliptical morphology with a concentrated, bright central bulge, indicative of an older stellar population. Its overall color leans towards the red end of the spectrum.

The secondary galaxy exhibits a more disk-like structure, possibly a spiral or lenticular galaxy seen at an oblique angle. It demonstrates a less concentrated central region and appears to be slightly bluer in color, suggesting the presence of younger stars or ongoing star formation.

There is evidence of tidal interaction between the two galaxies, possibly in the form of faint, extended features or distortions in their shapes, though the low resolution makes it difficult to confirm. The overall system is embedded in a faint halo of diffuse light. Given the color indices, absolute magnitudes and size, the interacting system appears to be massive. The estimated star formation rate suggests that the star formation is suppressed in the primary body, but there might be some ongoing star formation within the disk component.
