The galaxy presents as a relatively smooth, rounded object, lacking prominent spiral arm structures or a distinct central bulge. Its color profile indicates a dominance of older stellar populations, emitting strongly in the redder portions of the spectrum, with comparatively less blue light indicative of active star formation.

The overall structure suggests an elliptical morphology or a lenticular galaxy seen at a significant distance. There's no obvious sign of recent major merger activity, although subtle asymmetries or faint tidal features, if present, would be difficult to resolve at this image resolution. The apparent magnitude suggests a luminous object, implying a large stellar mass. The observed color and relatively smooth texture are consistent with a system where star formation has largely ceased, and the stellar population is dominated by older, redder stars.
