The object presents as a relatively smooth and concentrated elliptical galaxy with a redshift of approximately 0.37. The light profile indicates a central bulge that dominates the overall luminosity, exhibiting a distinct yellowish-orange hue. This coloration suggests a population of older stars. There appears to be very little visible star formation activity occurring. The galaxy appears fairly isolated, showing little to no evidence of major mergers or tidal disturbances. There may be a very small hint of a surrounding halo, but it appears very faint and without strong definition. The roundness of the object is pronounced.
