This galaxy presents as an elliptical or lenticular type. It exhibits a centrally concentrated bulge, decreasing in luminosity outwards towards what appears to be a faint, extended halo. The light distribution appears relatively smooth, with no obvious spiral arm structures or dust lanes visible at this resolution. There is a suggestion of some degree of disturbance in the outer regions of the galaxy. This disturbance could be a minor tidal interaction.

The galaxy displays a color profile consistent with a stellar population dominated by older, redder stars. The estimated redshift places this galaxy at a significant distance.
