The galaxy presents as a fairly smooth, elliptical-like object with a concentrated central bulge and a gradually fading halo. The core exhibits a yellowish-white hue, suggesting a population of older stars. There is little evidence of spiral arms or dust lanes, although a subtle disk-like feature may be present with a slight tilt. The light distribution is relatively uniform, indicating a lack of significant star formation regions. The galaxy appears undisturbed with no obvious signs of tidal interactions or recent mergers. The morphology suggests an evolved system, possibly a lenticular or early-type spiral galaxy nearing transition to an elliptical form, with a redshift indicating a considerable distance.
