The galaxy presents as a relatively compact object with a smooth, elliptical morphology. The overall color suggests an older stellar population, dominated by redder wavelengths, although there might be hints of bluer regions.

There's a noticeable lack of distinct spiral arms or a prominent disk structure. The light distribution is centrally concentrated, fading gradually towards the edges. The galaxy's shape appears more rounded than elongated, and the galaxy doesn't seem to be strongly disturbed, indicating no major ongoing or recent merger events. Some minor disturbances can not be ruled out.

The galaxy's redshift indicates that we are observing it at a substantial cosmological distance.
