The galaxy appears to be a relatively luminous elliptical or lenticular galaxy at considerable cosmological distance, evidenced by its small angular size and redshift. The light profile is dominated by a smooth, centrally concentrated bulge component, which is slightly elliptical in shape. The galaxy exhibits a color gradient, being notably redder in the central region and becoming subtly bluer in the outskirts. There may be a very faint, diffuse disk component, but its contribution to the overall luminosity is minimal. There is a slight asymmetry to the overall shape and distribution of light, possibly indicating a minor merger or tidal interaction.
